The galaxy presents a primarily smooth morphology, with a subtle suggestion of disk-like features. Its overall shape appears to be somewhere between round and elliptical. There are potential signs of minor disturbances in the galaxy's structure, suggesting a possible past interaction or merger event. The galaxy exhibits a color gradient, with a more yellow hue concentrated in the central region, potentially indicating a higher concentration of older stars in the core. The bluer light is more diffuse and is probably from areas where the stars are being born at a higher rate. It appears to be a late-type galaxy, possibly a spiral with a weak disk component. The estimated mass of the galaxy falls within the range of a typical galaxy, and it is forming stars.
