The galaxy presents as a slightly elongated, relatively smooth structure. There is a central bulge that appears luminous and concentrated. The overall color profile indicates a substantial population of older stars, likely dominating the light output. There is evidence of subtle disk-like features surrounding the bulge, though these structures appear less defined. There might be very small spiral arms but it is hard to tell with the resolution of the image. The disk shows an apparent tilt, producing the elongated appearance. A slight asymmetry is present, potentially indicating a minor past interaction.
