The galaxy appears as a moderately luminous, relatively smooth object. It displays a roughly elliptical morphology, with some deviation from perfect roundness; appearing slightly elongated. The galaxy's color profile suggests a dominant older stellar population, with a yellowish central concentration indicating a possible bulge. Faint hints of bluer light, potentially indicative of younger stars or low-level star formation, are present in the outer regions, although this is minimal. There is no clear evidence of spiral arms or a well-defined disk structure. No strong signs of ongoing major mergers or significant tidal disturbances are readily apparent, however, a faint extension on one side of the galaxy suggests a possible minor interaction. The overall structure points towards an evolved galaxy, potentially a lenticular or early-type spiral with subdued recent star formation.
