The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated luminosity profile. The overall shape is generally round. There is a distinct yellowish-orange hue to the central region, potentially indicating an older stellar population. The outer regions display a slightly bluer tint, suggesting the presence of some younger stars, although this is less pronounced than in spiral galaxies. There is no apparent disk structure, spiral arms, or significant dust lanes visible in this image. No signs of ongoing mergers or tidal disturbances are evident. The galaxy's morphology appears regular and undisturbed.
