The galaxy appears as a single, moderately bright object with a generally smooth morphology. The shape is predominantly round, with only a slight deviation toward elliptical. Color gradients are apparent, transitioning from a more yellow/orange hue at the core to a slightly bluer tint in the outer regions. The galaxy does not exhibit any obvious signs of spiral arm structure or strong dust lanes. There may be evidence of a very faint, diffuse halo surrounding the central region, but the low resolution makes this uncertain. There are no obvious signs of tidal disruption or an ongoing merger event. Overall, the galaxy’s smooth appearance and color profile suggests an elliptical or lenticular classification, likely dominated by an older stellar population. It is moderately massive, with moderate star formation activity.
