The galaxy presents as a centrally concentrated object with a generally smooth light distribution. Its overall shape appears to be neither perfectly spherical nor highly elongated, falling somewhere in between, leaning towards a more elliptical morphology. There's a suggestion of some disturbance or asymmetry in the outer regions, possibly indicating a past interaction or minor perturbation. The colour profile suggests a population of older stars, exhibiting a redder hue as compared to bluer star-forming regions typically seen in spiral arms, if present they are not visible. No clear spiral arm structure is discernible. There is no obvious presence of active galactic nuclei, bright point-like sources indicative of supermassive black hole activity at its core.
