The galaxy presents as a single, relatively concentrated object. Its overall morphology appears smooth and largely featureless, with a slight deviation from a perfectly circular shape. The light distribution suggests a centrally concentrated spheroid, possibly an elliptical galaxy. There is a subtle elongation, but no spiral arm structure is visible. 

The color profile indicates a redder hue in the central regions, transitioning to a slightly bluer tint at the edges. The lack of distinct features and the color gradient suggest a generally older stellar population, with possibly some ongoing star formation in the outer regions. There is no obvious evidence of significant dust lanes or strong tidal interactions.
