The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a concentrated, bright central bulge with a gradual decrease in luminosity outwards. The core is yellowish, suggesting a population of older stars. There is a subtle, diffuse disk component surrounding the bulge, discernible by a slight flattening of the galaxy's shape. There is minimal evidence of spiral arms or prominent dust lanes. The galaxy does not appear to be undergoing any major mergers, tidal distortions, or have any irregular features.
