The galaxy presents as a generally smooth, elongated structure. It appears to be an elliptical galaxy with a notable lack of distinct spiral arms or prominent dust lanes. The central bulge appears bright and concentrated, exhibiting a yellowish hue, suggesting an older stellar population dominating this region. Moving outward from the core, the light gradually fades into a bluer halo. The halo extension suggests a spheroidal distribution of stars beyond the main body. There are hints of slight disturbance or tidal features, potentially indicating minor interactions with other galaxies or internal dynamic processes, although no major merger is evident. Overall, the galaxy seems to be relatively evolved, with a declining star formation rate.
