The galaxy presents as a relatively smooth, elliptical-like structure. There is a centrally concentrated bulge, exhibiting a yellowish-orange hue, suggesting an older stellar population. The outer regions of the galaxy appear fainter and bluer, possibly indicating some degree of recent star formation or the presence of a younger stellar population in these regions. The galaxy lacks any prominent spiral arm structures. The overall morphology is consistent with an early-type galaxy undergoing little to no major merging activity. The elongation appears to be more in between a round and cigar shape. Based on the observed colors, it is likely that star formation rates are relatively low.