The galaxy presents as an elliptical morphology, elongated with a major axis estimated to be approximately 5 kpc in length. The light distribution appears smooth and centrally concentrated, indicative of an older stellar population. The core region exhibits a yellowish hue, potentially indicating the presence of evolved stars. The shape appears more cigar-like than round. There is no obvious evidence of spiral arms, a bar, or significant dust lanes, which are features commonly associated with spiral galaxies. The outer regions of the galaxy gradually fade into the background, suggesting a diffuse stellar halo. There are no readily discernible signs of recent or ongoing mergers or tidal disturbances based on the image alone.
