The galaxy presents a predominantly smooth morphology. It appears nearly symmetrical, with no strong spiral arm features or bar structure visible. The light is centrally concentrated, with brightness decreasing gradually towards the outer edges. The central region exhibits a bright, possibly older stellar population indicated by the whiter and slightly yellow hue. There's some subtle bluer tinting appearing asymmetrically on one side of the central bulge, potentially indicating ongoing star formation. The galaxy's overall shape leans towards being slightly elongated, not perfectly circular. There is no evidence of major mergers or significant tidal disturbances affecting the galaxy's form.
