The galaxy appears to be an elliptical galaxy with a smooth, concentrated light profile, exhibiting a high degree of symmetry. Its color suggests a population dominated by older stars, with a relatively low ongoing star formation rate. There is a subtle color gradient, with the central region appearing slightly more yellow compared to the outer regions, which have a faint bluish tinge. This could indicate a difference in stellar populations or metallicity between the core and the outskirts. The galaxy shows no obvious signs of spiral arms or a prominent disk. There is a slight suggestion of minor tidal disturbance or interaction with another galaxy, which is indicated by a faint trail of matter or a slight asymmetry in the outer halo of the galaxy. The galaxy is neither perfectly spherical nor highly elongated.
