The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal in shape. There is a concentration of light toward the center of the galaxy, indicating a significant bulge component. The light distribution suggests that the galaxy is more "in between" rounded and cigar shaped rather than perfectly round.

There is an indication of possible minor disturbances within the galaxy's structure, which may be related to ongoing or past interactions with smaller satellite galaxies. The galaxy exhibits a color gradient, transitioning from a bluer tint towards the outer regions to a redder hue near the core, which may be indicative of aging stellar populations concentrated in the galaxy's center and ongoing star formation in the outer regions. The overall light profile suggests a system dominated by older stars, but with a non-negligible population of younger stars in the outer regions. The galaxy is observed at a redshift, suggesting that it is at a significant cosmological distance.
