The galaxy appears as a smooth, elongated structure, likely an elliptical galaxy or a lenticular galaxy viewed edge-on. The light distribution is concentrated toward the center, with a gradual decrease in intensity outwards. There is no apparent spiral arm structure or distinct features, suggesting it is a relatively quiescent system in terms of star formation. The galaxy exhibits a redder color, which may be due to an older stellar population. Some minor tidal disturbances are possibly present on the edges, but it has probably not experienced a major merger. 
