The galaxy presents an elongated, cigar-like morphology, suggesting it is an elliptical galaxy viewed nearly edge-on. The light distribution appears relatively smooth, with a gradual decrease in intensity from the center outwards. There is a subtle color gradient, with a slightly bluer hue towards the edges compared to the central bulge, potentially indicating the presence of some younger stellar populations in the outer regions. No distinct spiral arm structures or prominent dust lanes are discernible, further supporting its classification as an elliptical galaxy. There are no signs of any major mergers or significant tidal disturbances.