The galaxy presents as a relatively smooth, elliptical form. Its color profile suggests a dominant population of older stars, giving it a yellowish-white hue concentrated toward the galactic center. There is a noticeable lack of distinct spiral arm structures or significant dust lanes. The galaxy appears to be quite uniform, with a smooth transition from the bright, compact core to the more diffuse outer regions. The overall shape leans towards a rounded morphology with a slight elongation, but not distinctly cigar-shaped. There's no obvious visual evidence of ongoing major mergers or tidal disturbances affecting its structure. The observed characteristics are consistent with an early-type galaxy, possibly an elliptical or lenticular, exhibiting little current star formation activity.
