The galaxy appears to be a relatively smooth, elliptical-type galaxy, exhibiting a generally spheroidal morphology. It presents a concentrated central bulge region that is bright and dominates the overall luminosity. There are no discernible spiral arm structures or a prominent disk. The galaxy exhibits a color gradient, with the core showing a slightly redder hue compared to the more extended outer regions which appear subtly bluer. No significant tidal features or signs of recent major merger events are immediately apparent, although there may be some minor irregularity in its outer isophotes suggesting past interaction or minor disturbance. The galaxy's light profile appears well-behaved, without significant asymmetry or strong dust lane obscuration. The stellar population seems to be a mix of older, redder stars in the core and a younger, bluer population towards the outskirts, suggesting ongoing, but not intense, star formation activity. The overall structure suggests a gravitationally relaxed system, having undergone significant dynamical evolution.
