The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, exhibiting a high degree of roundness with minimal deviation from a spherical shape. There is little evidence of distinct spiral arms or a prominent disk structure. The galaxy exhibits a color profile that is centrally reddish-yellow, fading outward to a pale blue hue. There are no obvious signs of on-going major merger activity or tidal disturbances, although a subtle asymmetry in the outer isophotes might suggest a past minor interaction or accretion event. The galaxy appears to be relatively isolated in its immediate environment, with no other comparably sized galaxies in close proximity. Given the apparent smoothness and color profile, the galaxy is potentially a relatively massive and evolved system, with an older stellar population. Star formation activity is not readily apparent.
