The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge. The light profile is centrally concentrated, with a gradual decrease in brightness toward the outer edges. The core region has a yellowish hue, possibly indicating an older stellar population. There is a subtle bluish tint in the outer regions, indicative of ongoing star formation. Based on these properties, it seems like this galaxy is currently dominated by older stars. It does not appear to show signs of significant tidal disturbances or interactions with other galaxies. The shape is mostly round.
