The galaxy presents as a relatively smooth, elliptical-shaped object. It appears highly rounded. There is no obvious spiral arm structure or distinct disk features visible. The galaxy exhibits a subtle color gradient, with a slightly bluer hue at the center that transitions to a redder color towards the outer edges. This may indicate some ongoing star formation localized to the core, although the overall morphology suggests a galaxy dominated by older stellar populations. There is no clear evidence of a major merger event. There is some indication of a minor disturbance in the galaxy's overall structure, but no major signs of tidal features.
