The galaxy appears as a centrally concentrated object, with a smooth, somewhat elliptical morphology. There is a slight elongation, but it is mostly round. The central region exhibits a brighter, more condensed luminosity profile, likely indicating a bulge. There is some asymmetry in the outer regions, perhaps suggestive of minor disturbances or interactions. The overall color profile suggests the presence of a relatively older stellar population, with subtle hints of ongoing star formation. Though the galaxy is generally smooth, there is a slight indication of a disk-like structure.
