The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution suggests an older stellar population, exhibiting a predominantly reddish-yellow hue. There's little evidence of distinct spiral arms or significant dust lanes; the overall appearance is quite homogenous. The shape appears mostly round with some elongation. There are some indications of minor disturbances in the outer regions, suggesting recent or ongoing gravitational interactions. There's a possible indication of a tidal tail or a very faint stream of stars emanating from the main body, but it's difficult to confirm with the available resolution. Overall, this galaxy appears to be a massive, evolved system with a relatively low star formation rate.
