The observed galaxy presents an overall elongated morphology. The central region exhibits a bright, concentrated luminosity, suggesting a prominent galactic nucleus or core. The light distribution appears relatively smooth throughout, hinting at a lack of well-defined spiral arm structures or significant dust lane features.

The color gradient within the galaxy seems to indicate a bluer hue in the outer regions gradually shifting toward redder tones toward the center. This may be indicative of younger stellar populations residing in the outskirts, while older, redder stars concentrate toward the galactic center.

There is a hint of a minor disturbance or asymmetry in the galaxy's overall shape. This could be from a slight tidal interaction, or a minor recent merger event with a smaller object. Though the galaxy is generally smooth, there are very faint wisps or tails on one side of the object.
