The galaxy appears to be a relatively smooth, elliptical type. It exhibits a central bulge that dominates the overall light profile. The light from this central region is yellowish-white, suggesting an older stellar population. Moving outward from the center, the light gradually fades into a bluish hue, indicating the presence of some younger, bluer stars, but not significant star formation.

The galaxy's shape is somewhat elongated, but it lacks any obvious spiral arm structures or significant dust lanes. The smooth light distribution suggests a relatively relaxed system. There may be some minor disturbances present, but they don't dramatically impact the overall morphology. There is no visual evidence of a recent or ongoing major merger.
