The galaxy presents as a relatively smooth object with a concentrated central bulge. The shape approximates a rounded form, with a slight deviation towards an intermediate elliptical classification, though not elongated. There is no prominent disk structure discernible. The galaxy's light profile appears uniform, showing no spiral arms, bars, or other features of strong active star formation. Given the overall morphology and color indices, the galaxy appears to be a relatively evolved system, potentially dominated by an older stellar population with low rates of current star formation. There is some evidence of minor disturbances in the outer regions, but the galaxy, on the whole, does not seem to be currently undergoing a major merging event. 
