The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a well-defined disk structure. The light profile seems to be centrally concentrated, with a gradual decrease in brightness from the core outwards. The galaxy exhibits a moderate degree of roundness, appearing nearly circular in shape. There is no obvious evidence of ongoing or recent major merger activity, though a very slight asymmetry in the outer regions could suggest a minor interaction in its past. The color appears relatively uniform across the galaxy, suggesting an older stellar population. The low rate of star formation is consistent with the overall redder color. Based on the size and apparent magnitude, it seems to be a fairly small galaxy.
