The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge that fades gradually into the outer regions. The core exhibits a yellowish hue, potentially indicating an older stellar population. The surrounding halo appears more diffuse and bluish, possibly signifying a low level of ongoing star formation. No prominent spiral arms or significant dust lanes are discernible. The overall morphology suggests a lack of major recent merger events, with the galaxy appearing largely undisturbed. The galaxy has a low star formation rate. The estimated mass is within the range of a typical elliptical galaxy.
