The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a high degree of central concentration. The light profile appears to decrease gradually from the bright nucleus outwards, with no apparent spiral arm structures or prominent dust lanes visible. The galaxy's shape is elongated, though it is somewhere between round and cigar shaped, indicating some degree of flattening. There are no clear signs of ongoing major mergers or strong tidal disturbances. The overall color seems relatively homogenous and lacks significant blue components, suggesting a dominant population of older stars and a comparatively low star formation rate.
