The galaxy presents as a diffuse, somewhat amorphous structure with a centrally concentrated luminosity. It appears relatively smooth, lacking sharply defined spiral arms or a prominent bar. The light distribution suggests a roughly elliptical morphology, though not perfectly spherical.

Color gradients are subtle, with a tendency towards bluer hues at the outer edges of the galaxy and a slightly redder, more yellow tint towards the center. This could indicate ongoing or recent star formation in the outer regions and an older stellar population concentrated in the core.

There is a suggestion of some minor disturbance. The galaxy's light is not evenly distributed, with some subtle asymmetry visible. A possible interaction or minor merger event with a smaller companion in the past cannot be ruled out, though the galaxy does not appear to be undergoing a major, disruptive merging process.
