The galaxy presents as an elliptical morphology, with a smooth, featureless appearance. The light distribution suggests a central bulge that dominates the overall luminosity. The galaxy exhibits a slight elongation, appearing cigar-shaped. Color gradients suggest the presence of older stellar populations, particularly in the central regions. Some bluer hues are visible in the outer edges indicating areas of star formation. No significant dust lanes or spiral arm structures are discernible. The galaxy is relatively isolated, without obvious signs of ongoing major interactions or mergers.
