The galaxy appears as a lenticular, cigar-shaped object with a smooth, diffuse light distribution. A bright central bulge dominates the core, transitioning into a fainter, elongated disk extending along the major axis. The outer regions of the disk show a subtle blue tinge, possibly indicative of ongoing or recent star formation. The overall color suggests a relatively older stellar population within the dominant bulge component. There is no apparent evidence of spiral arm structure or significant dust lanes visible in this image, and no interactions or major disturbances, such as tidal tails, are observed. The galaxy displays a relatively regular morphology.
