This galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that transitions smoothly into a more diffuse outer region. The galaxy displays a generally rounded morphology. The color profile suggests a population of older stars, indicated by the yellowish-orange hue, with limited evidence of significant ongoing star formation. There is no distinct disk or spiral arm structure visible. The overall symmetry of the galaxy is not significantly disrupted, suggesting that it is not currently undergoing a major merger event.
