The galaxy presents a largely smooth morphology, appearing elliptical in shape with a slight elongation. There is no discernible spiral arm structure, and no obvious bar feature. The galaxy's light is centrally concentrated, with a gradual decrease in intensity outwards. The color profile suggests a population of older stars, with a redder hue dominating the core and extending throughout the galaxy's visible extent. There may be some minor disturbances based on subtle irregularities in its outer regions, but it doesn't appear to be undergoing a major merger or strong tidal interaction. The estimated size suggests it is a moderately sized galaxy, not exceptionally large or small.
