The galaxy presents as a somewhat elliptical, unresolved object. It exhibits a centrally concentrated luminosity profile, suggesting a large stellar bulge. The core appears to be a yellow-orange hue, likely indicative of an older stellar population. There is evidence of a bluer, diffuse halo or outer disk surrounding the central bulge; though the resolution limits a precise morphological classification, it seems to have a smooth appearance with no clear spiral arm structure visible. The relatively uniform color gradients suggest a lack of significant ongoing star formation in the central regions, though some star formation is likely occurring in the outer regions. There is no apparent sign of a tidal disturbance.
