This galaxy appears to be a relatively smooth, elliptical galaxy. The core exhibits a concentrated, bright luminosity, indicative of an older stellar population. The isophotes appear generally round, with a slight elongation. There is no apparent disk structure or prominent spiral arms. Faint, diffuse light extends outward from the central region, suggesting a spheroidal component. There is a subtle indication of some minor tidal disturbance or interaction based on the asymmetry and faint extensions present. Overall, the galaxy exhibits characteristics consistent with a mature galaxy with a relatively low ongoing star formation rate.
