The galaxy presents as a moderately sized, elliptical or lenticular system. It exhibits a centrally concentrated luminosity profile, fading towards the outer regions. No spiral arm structures are discernible within the image. The galaxy appears relatively smooth in texture, with no obvious dust lanes or prominent star-forming regions. The colour profile is generally consistent across the galaxy, indicating a relatively homogenous stellar population. There is no strong evidence of any ongoing mergers or tidal disturbances. The central region may possess a subtle brightening, possibly indicative of a galactic nucleus.
