The galaxy presents as an elliptical morphology, exhibiting a smooth light distribution with no apparent spiral arm structure or prominent dust lanes. The core region is bright, with a yellow hue suggestive of an older stellar population. The galaxy is not perfectly spherical, displaying a slight elongation, tending toward an in-between roundness, but not significantly cigar-shaped. There is no obvious evidence of ongoing major or minor mergers, tidal tails, or other signs of significant gravitational disturbance. Color gradients suggest a mild radial variation in stellar populations, with the central region possibly more metal-rich or containing a higher proportion of older stars compared to the outer regions, where there is a very faint blue tinge, indicating recent star formation.
