The galaxy exhibits a generally smooth morphology, with a slightly elongated shape that is somewhere between round and cigar-shaped. The light distribution is concentrated, showing a bright central region that fades gradually towards the edges. There's also some evidence of internal structure or possible faint spiral arms or disk. The galaxy appears relatively isolated, showing no obvious signs of a major merger, although a minor disturbance cannot be entirely ruled out given its slightly irregular shape. Color gradients indicate that the central part of the galaxy is relatively older and redder, potentially indicating a population of older stars, while outer regions may show bluer colors, hinting at more recent star formation activity.
