The galaxy appears as a relatively smooth, centrally concentrated object with an elliptical morphology. The light distribution suggests a single, dominant component, lacking prominent spiral arms or a distinct disk structure. There may be a slight asymmetry. The color profile indicates a generally older stellar population with a reddish hue, possibly due to a lower star formation rate and dust content. Based on the color profile, this is likely an older galaxy. There are no obvious signs of major mergers or tidal disturbances.
