The galaxy presents a morphology consistent with an elliptical type, exhibiting a generally smooth light distribution. The central region displays a high degree of luminosity, with a gradual decrease in brightness toward the outer edges. The overall color profile indicates a population of older stars, contributing to its redder hue. There is a slight asymmetry in the distribution of light, particularly at one end of the major axis. This may indicate a minor disturbance or tidal feature, but a more detailed spectral analysis would be needed to confirm. The galaxy does not appear to have a distinct disk component or spiral arms, further supporting classification as an elliptical galaxy. The size is on the smaller size, appearing compact.
