The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. The light is primarily yellowish-white at the core, suggesting an older stellar population. There is a gradual transition from the bright core to a fainter, more diffuse outer region, which exhibits a bluer hue. This suggests the presence of some younger stars. The galaxy lacks any obvious spiral arm structure or prominent dust lanes. There's no evidence of a major ongoing merger, although some minor irregularity in the outer halo cannot be ruled out at this resolution. Overall, it appears to be a massive galaxy with moderate star formation.
