The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, concentrated bulge that dominates the central region. There is little evidence of defined spiral arms or significant dust lanes. The galaxy appears somewhat elongated with a cigar-shaped morphology. A diffuse halo surrounds the central bulge, gradually fading into the background sky. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central regions. The outer regions appear slightly bluer, possibly indicating a small amount of recent star formation. Overall, the galaxy appears relatively isolated with no apparent signs of major interactions or mergers.
