The galaxy presents a morphology that appears to be somewhere between smooth and disk-like. The central region exhibits a bright, concentrated bulge that dominates the overall luminosity profile. The bulge appears to be slightly elongated rather than perfectly spherical. Fainter, diffuse light extends outwards from the bulge, forming a less defined disk-like structure. There is a noticeable lack of well-defined spiral arms.

There is evidence of minor disturbances or tidal features. Specifically, there are redder knots or regions located on either side of the main galactic body, these could be remnants of a minor interaction with another galaxy, or could indicate an active star forming region. The overall color of the galaxy appears relatively uniform, trending towards redder hues, especially in the knots, which suggests an older stellar population and suppressed star formation throughout the primary disk.
