The galaxy appears to be a relatively smooth, centrally concentrated system. Its color profile indicates a dominant population of older stars, with a yellowish hue. There is a subtle extension of light suggesting a disk-like structure. The disk exhibits slight bluer patches which may represent pockets of localized star formation. Overall, the galaxy's morphology leans towards an elliptical or lenticular type. There are some possible signs of minor disturbance in the galaxy's morphology, indicating a possible past or ongoing interaction or merger event. However, its large central bulge is the dominant feature.
