The galaxy presents an elliptical morphology. The light distribution appears smooth and centrally concentrated, exhibiting a spheroid shape. The core of the galaxy displays a yellowish hue, suggestive of an older stellar population. Fainter bluish light surrounds the central region, possibly indicating the presence of a younger, though still minimal, stellar population in the outer areas. There is no discernable spiral arm structure. The shape is elongated, being more cigar-shaped than round. There are no obvious signs of tidal disturbances or ongoing mergers. The galaxy does not appear to be actively undergoing significant star formation.