The galaxy appears as a centrally concentrated elliptical or lenticular system. It presents a smooth, generally featureless morphology with a bright core. The light profile exhibits a gradual fall-off from the nucleus to the outer regions. There is minimal indication of spiral arms or prominent dust lanes. The galaxy's overall shape is roughly elliptical, with a slight preference towards a more rounded appearance, though some elongation cannot be ruled out. There is no obvious sign of ongoing or recent merger activity, though slight irregularities in the outer halo could point towards a possible minor disturbance. The system appears to be relatively quiescent in terms of star formation activity. The galaxy exhibits a color index suggesting a population of older, redder stars, consistent with a post-starburst or passively evolving system.
