The galaxy presents a largely smooth, elliptical morphology. The light distribution suggests a centrally concentrated bulge, with a gradual decline in luminosity towards the outer edges. It appears slightly elongated, exhibiting a cigar-like shape. There is no readily apparent dust lane or spiral arm structure discernible. The overall color profile suggests a relatively older stellar population. The lack of distinct features indicates minimal ongoing star formation activity. There is no morphological evidence to suggest any recent or ongoing merger events.
