The galaxy presents a largely smooth, elliptical morphology. The central bulge is a prominent feature, exhibiting a bright, concentrated luminosity gradient, indicative of a high stellar density.  There is a subtle gradient in color from the center outwards, with the core exhibiting a yellower hue, possibly indicating a population of older stars.  Faint extensions surrounding the central region suggest a diffuse halo or envelope, though no distinct spiral arm structure or prominent dust lanes are visible. The overall shape suggests minimal recent or ongoing major merger activity, and there is no evidence of tidal tails or streams. The galaxy has a moderate size, extending across a few arcseconds in this image.
