The galaxy presents as a moderately bright, somewhat diffuse object with a dominant central bulge. The overall morphology is elliptical, though the shape is not perfectly regular. There is evidence of some disk structure. The galaxy displays a redder hue in the central regions, potentially indicating an older stellar population and diminished star formation. Fainter, bluer regions are observed further away from the galaxy center, suggestive of more recent star formation. The galaxy exhibits an intermediate roundness, leaning towards more elongated than completely round. The structure is mostly smooth, but some low-level disturbances are apparent, suggesting a potential past or ongoing interaction. There may be the presence of an active galactic nucleus in the center. The galaxy shows no strong spiral arm structure or prominent dust lanes.
