The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile indicates a population of older stars, contributing to its yellowish-orange hue. There is minimal evidence of spiral arm structures or significant dust lanes. The object exhibits a high degree of circular symmetry and lacks any obvious signs of major tidal disturbances or ongoing merger activity. Faint, diffuse light extends from the central region, suggesting a gradual decline in stellar density towards the galaxy's outer regions. Overall, the galaxy appears to be a well-defined, relatively quiescent system.
