The galaxy presents as a centrally concentrated object with a generally smooth morphology. It exhibits an elliptical shape, appearing more round than elongated. The color profile suggests an older stellar population, trending toward redder hues. There's a subtle disk-like structure, possibly with weak spiral arms. Indications are present of minor disturbances, but no significant merging is visible. Based on its color and smoothness, it is likely a galaxy undergoing moderate star formation.
