The galaxy presents as a relatively smooth, elliptical structure. The light is concentrated toward the center, with a gradual decrease in intensity moving outward. The color profile suggests an older stellar population, with a yellow-red hue dominating the central region, and some bluer components in the surrounding regions. There is no strong evidence of spiral arms or significant dust lanes. The overall shape indicates an elliptical morphology, with a slightly elongated or cigar-shaped appearance. There are no obvious signs of ongoing major merging events. The galaxy is estimated to be a moderate mass galaxy with extremely low star formation rate.
