The galaxy presents an elongated morphology, appearing as a flattened spheroid. Its central region exhibits a bright, concentrated luminosity, indicative of a prominent galactic nucleus or bulge. The primary color of this central region is a strong yellowish-orange, potentially suggesting an older stellar population dominating this area.

Extending outwards from the core are fainter, more diffuse arms or disk-like structures. These structures seem somewhat disrupted or irregular in shape, showing no clear, well-defined spiral arm pattern. Their color shifts towards greenish-yellow and possibly a hint of redder hues, which could indicate regions of ongoing star formation or the presence of dust lanes.

Overall, the galaxy's morphology suggests a possible transition between a spiral and elliptical type, or a galaxy that has undergone recent disturbances. The light distribution is uneven and patchy, which might be the result of a minor merger event or tidal interactions. The relatively smooth appearance doesn't exclude the possibility of underlying features that cannot be clearly distinguished at this resolution.
