The galaxy appears to be an elliptical type, characterized by a smooth, centrally concentrated distribution of light. It exhibits a generally round shape, with no obvious spiral arms or disk features. The central region is bright and yellowish, suggesting an older stellar population. The outskirts of the galaxy fade gradually into the background, with no sharp edges or distinct halo. There is little evidence of ongoing star formation activity and no signs of recent or ongoing major merger events. Faint disturbances may be present, although they are not obvious. The galaxy's overall appearance is consistent with a relatively evolved system dominated by older stars.
