The galaxy presents as a moderately bright, elongated spheroid with a smooth light distribution. The central region appears somewhat more concentrated, gradually fading towards the edges. The galaxy exhibits a yellowish hue overall, suggesting a population of older stars, though it is still actively forming new stars. No distinct spiral arms or bar structures are discernible in the available image. The isophotes appear relatively undisturbed, lacking evidence of major mergers or strong tidal interactions. There is a slight indication of a subtle, minor disturbance in the galaxy's shape, possibly indicating a small past interaction. The galaxy's overall shape is somewhere in between round and cigar-shaped.