The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. There are no prominent spiral arms or obvious features indicative of active star formation within the visible light spectrum. The galaxy appears roughly circular in shape, with a slight elongation that could suggest a mild cigar shape. There are no significant signs of ongoing major mergers or tidal disturbances affecting the galaxy’s morphology, though some minor asymmetry is present. The color profile suggests a population of older stars and a lack of significant dust lanes or prominent HII regions. The faint outer regions of the galaxy are indistinct, appearing as a diffuse halo surrounding the bright core.
