The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The light profile appears relatively uniform with a gradual decrease in intensity from the core outwards. There are no prominent spiral arms, bars, or dust lanes visible in this image. It has an average mass estimate in terms of stellar mass.

The color is observed to be slightly redder, suggesting a population of older stars and relatively low ongoing star formation. Star formation is present, although not at a high rate. The galaxy's shape is approaching round, without any distinct elongation, though it is not perfectly circular. There is no strong evidence of a major ongoing merger or tidal disturbance, though minor disturbances or interactions cannot be ruled out.