The galaxy exhibits a generally smooth morphology, displaying a predominantly spheroidal or elliptical shape. It shows little to no apparent spiral arm structure. The overall color appears to be on the redder side, indicating a population of older stars and a relatively low rate of current star formation. The object displays a somewhat elongated form, with a hint of disturbance in its structure, which suggests a possible past interaction or minor merger event. There is no strong evidence of an ongoing major merger, though the possibility of a minor disruption cannot be ruled out. The galaxy presents a concentrated core, but no distinct disk component is readily discernible in this image.
