The galaxy presents as a relatively smooth, somewhat rounded object. The central region exhibits a bright, concentrated luminosity, suggesting a significant stellar population density. Surrounding this central bulge is a fainter, more diffuse halo. There is an indication of some disturbance in the galaxy's morphology, with some irregular features suggesting a possible interaction or ongoing merger event. The galaxy has a generally redder color, potentially indicative of an older stellar population and lower current star formation rate.
