This galaxy appears as a faint, relatively small, and somewhat diffuse object. Its overall color suggests a mix of stellar populations, with a possible redder core and bluer outer regions. There is not a clear disk structure; instead, a smoother distribution of light is observed. Based on the slight asymmetry and fuzzy edges, there could be some evidence of tidal disturbance or recent interactions with a smaller galaxy. There is no distinct nucleus, and there appears to be very little ongoing star formation. Overall, the galaxy shows characteristics of being a passive system, though some subtle irregularities hint at some low level of gravitational interaction.