The galaxy presents as an elliptical-like morphology, exhibiting a generally smooth and concentrated distribution of light. There appears to be a luminous central bulge or core region that transitions smoothly into the outer regions of the galaxy. The galaxy is elongated, appearing more "in-between" round and cigar shaped than either extreme. Faint hints of structure suggest some minor disturbances in the galaxy's form but it does not appear to be undergoing a major merger event. The color profile exhibits a yellowish-white core with a gradient to bluish hues on the outer edges. This color distribution suggests the presence of an older stellar population dominating the central region, with a relatively lower presence of younger, bluer stars in the outlying disk. 
