The galaxy presents a generally smooth and rounded morphology. The central region exhibits a concentrated luminosity profile, appearing bright and slightly yellowish, suggesting a higher density of older stellar populations. There is little evidence of spiral arm structures or significant dust lanes. The overall light distribution suggests an elliptical galaxy or a lenticular galaxy viewed face-on. A slight asymmetry is visible in the outer regions of the galaxy, indicating the possibility of a minor disturbance. Based on the color indices, the galaxy appears to have moderate star formation activity, although the dominant stellar population seems to be older. No signs of a major merger event are immediately apparent from the image.
