The galaxy appears as a distorted disk with a central bulge that is not well-defined. The color gradient transitions from a bluer hue at the edges, suggestive of younger stellar populations, to a redder tone within the central regions, indicating the presence of older stars. There are several bright spots spread throughout the galaxy, potentially indicating active star-forming regions or luminous clusters. The overall structure hints at possible gravitational interactions or a recent merger event, suggested by the irregular shape and lack of a clear spiral arm structure. A dust lane is not clearly visible but could be obscured due to the angle of observation. There is a chance that this is a galaxy in the late stages of a merger, as it appears to be in an intermediate state of disorder.