The galaxy presents as a smooth, elliptical-like structure with a noticeable central bulge. Its overall shape is elongated, exhibiting a cigar-like morphology rather than a perfectly circular one. There appears to be a gradual color gradient from the center outwards; the core exhibits a yellowish hue, suggestive of an older stellar population. Moving outward from the core, the color transitions toward a slightly bluer, fainter luminosity, indicative of some younger stars or differing stellar populations within the galaxy's outer regions. The light is distributed relatively smoothly, showing no apparent strong spiral arm structures or significant dust lanes. There is no sign of ongoing major mergers or tidal disturbances. However, a slight asymmetry in the outer regions could suggest a minor past interaction.
