The galaxy presents as a well-defined, elliptical structure with a smooth light distribution. The morphology appears largely undisturbed, showing no signs of a major merger or tidal disruption. The central region exhibits a concentrated, brighter core, suggesting a higher density of stars and potentially a supermassive black hole.

The galaxy's color profile indicates a redder core transitioning to a slightly bluer outer halo. The redder core is indicative of an older stellar population, while the bluer halo suggests the presence of younger, hotter stars. The galaxy exhibits a degree of elongation, appearing cigar-shaped. Based on the observed characteristics, this galaxy is likely a massive, passively evolving elliptical galaxy with a relatively low star formation rate.
