The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually diffuses outwards. The shape is elongated, appearing somewhat cigar-shaped rather than perfectly circular. There are no obvious signs of spiral arm structure or significant dust lanes visible within the image. The galaxy's color profile appears consistent throughout with a slightly yellowish/reddish hue, indicative of a population of older stars. No major disturbances or signs of ongoing merger activity are readily apparent, though a minor asymmetry or subtle feature could possibly be present upon further investigation. The galaxy appears isolated, with no other galaxies in close proximity that might suggest tidal interactions. Overall, the galaxy gives the visual impression of being a mature, quiescent system.
