The galaxy presents as an elliptical structure, exhibiting a smooth light distribution characteristic of elliptical galaxies. The central region appears very bright, with a concentrated luminosity suggesting a significant stellar population. The galaxy's profile is more elongated than circular, but not extremely so. There are suggestions of faint, extended material surrounding the main body, though the edges are indistinct. No distinct spiral arms or prominent dust lanes are visible. There is a slight hint of bluer light at the very outskirts of the galaxy, but its overall color is indicative of a population of older stars. No significant signs of ongoing major merger activity or tidal disruption are apparent.
