The galaxy appears to be a relatively smooth, elliptical-type galaxy, with a high degree of central concentration. There is a notable lack of distinct spiral arm structures or prominent dust lanes. The galaxy exhibits a generally rounded morphology, though it does not appear perfectly spherical. The color profile suggests an older stellar population, with a yellow to reddish hue dominating the central regions. Some minor disturbances might be present in the outer regions, but the bulk of the galaxy seems largely undisturbed. Overall, this galaxy presents as a fairly massive system with a low ongoing star formation rate.
