The galaxy presents as a somewhat smooth, rounded structure, although not perfectly spherical. A central, bright bulge is visible with a yellowish hue, suggesting a population of older stars. Fainter, bluer light extends outward from the central region, possibly indicating some ongoing star formation. A small, distinct reddish patch is observed on one side of the bulge, which could be indicative of an HII region or a region of intense star formation heavily obscured by dust. There is a slight asymmetry or minor disturbance in the overall structure, hinting at a possible past interaction or merger event. Overall, this galaxy appears to be an intermediate-mass system with a moderate level of star formation activity.
