This galaxy presents a generally smooth, elliptical morphology. It appears to be moderately flattened, displaying an intermediate ellipticity, trending towards a cigar-like shape. The central region exhibits a concentrated luminosity, suggesting a prominent bulge component. The color profile indicates a population of older stars in the core, with a shift toward slightly bluer hues in the outer regions. There's no strong evidence of significant ongoing star formation, and the galaxy does not show signs of a major merger. However, there is a small irregular object or region that could be a minor disturbance. This could be a tidal tail or perhaps a satellite galaxy undergoing disruption, indicating possible interaction with its environment.
