The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity towards the outer regions. The dominant color is yellow-orange, suggesting an older stellar population. There is little to no evidence of spiral arms or prominent dust lanes, which implies a lack of active star formation. The galaxy appears to be fairly round, with no significant elongation or tidal features visible. No major disturbances or ongoing mergers are apparent in this observation, hinting at a gravitationally relaxed system. The estimated size corresponds to approximately 6 kpc across, assuming the data is accurate.