The galaxy presents an elliptical morphology, displaying a centrally concentrated luminosity profile, suggesting a relatively smooth distribution of stars within. The light is strongest in the center, gradually decreasing at the edges, with no obvious spiral arm structures or dust lanes visible. Color appears to be fairly uniform across the galaxy, with a slight redder hue overall, indicating an older stellar population. The galaxy appears relatively isolated. Evidence of tidal tails or other major distortions suggesting ongoing or recent major merger events is minimal. There is a subtle asymmetry to the light distribution, possibly indicating a minor interaction, or the presence of faint, unresolved features.
