The galaxy presents a generally smooth, elliptical morphology with a slightly elongated, but not cigar-shaped, appearance. A dominant central bulge is evident, characterized by a yellowish hue, potentially indicating an older stellar population with lower rates of star formation. There are hints of a surrounding disk or extended structure, displaying a more greenish-blue color, suggestive of the presence of younger, hotter stars and ongoing star formation within the galaxy. There is a slight asymmetry in the outer regions, possibly due to a minor gravitational interaction or past merger event that hasn't drastically disrupted the overall smooth structure. The galaxy does not appear to be undergoing any major merger or significant disturbance based on the data.
