The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The color profile is somewhat red, indicative of an older stellar population with lower ongoing star formation. There is little evidence of spiral arms or significant disk structure; the light appears to be fairly uniform across the galaxy's body, with only a slight concentration towards the center. Based on the smoothness of the galaxy, there doesn't seem to be a significant ongoing merger or interaction event distorting its morphology. The overall appearance suggests a gravitationally settled system dominated by older stars.
