The galaxy appears as an elliptical-type system, exhibiting a smooth, centrally concentrated morphology. The central region displays a yellowish hue, indicative of an older stellar population. Moving outwards from the core, the light gradually diminishes with no signs of prominent spiral arms, dust lanes, or active star formation regions readily discernible. The galaxy's shape is mostly in between round and cigar shaped. There are no clear signs of any recent major merger activity or tidal disturbances, although it is difficult to tell. The galaxy appears mostly undisturbed.
