The galaxy presents as a small, relatively faint object with a compact appearance. It is characterized by a smooth light distribution, lacking any prominent spiral arms or distinct morphological features. The color profile suggests a moderately red hue, indicating a likely older stellar population and/or significant dust content. There is no strong evidence of a bulge or disk structure visible in this image. The overall morphology leans towards an elliptical or lenticular classification, with a slight possibility of a compact spiral galaxy viewed at a high inclination. There is little indication of ongoing major mergers, tidal disturbances, or intense star formation activity within the galaxy.
