The galaxy presents a largely smooth morphology, with a centrally concentrated bulge that dominates the overall light profile. The radial color gradient suggests a potential variation in stellar populations, with the central region appearing more yellow-orange and the outer regions exhibiting a greenish hue. A faint disk component may be present, but it is difficult to definitively confirm due to the galaxy's orientation and the prominence of the central bulge. There is no significant evidence of spiral arms, bar structures, or major disturbances indicative of recent mergers. A slight irregularity in the outer isophotes on the periphery of the galaxy suggests potential minor interactions or accretion events in the past. Overall, the galaxy appears to be an elliptical or lenticular type, characterized by its smooth light distribution and dominant bulge.
