The galaxy appears to be an elliptical galaxy, displaying a generally smooth, concentrated light profile. The galaxy's light is yellowish in its core, suggesting a population of older stars. There is a slight color gradient from the center to the outer regions, with the outer regions appearing slightly bluer. Based on the observed morphology, the galaxy shows no distinct spiral arm structures or major disturbances indicative of ongoing major mergers, but there is some evidence of a minor disturbance. The elongated shape is in between round and cigar-shaped. The galaxy is relatively compact and appears to have a low rate of star formation based on its color. The estimated size is relatively small. The overall structure suggests a mature, relatively quiescent system that may have undergone some recent minor interaction.
