The galaxy exhibits a somewhat elongated morphology. A central bulge is discernible, with evidence of a possible disk structure extending outwards. The light distribution is not entirely uniform, showing irregularities that could suggest either internal structures or ongoing interactions. The color gradient across the galaxy indicates varying stellar populations. In the central region, a concentration of redder hues is observed, potentially indicative of older, cooler stars. The outer regions display a bluer tint, suggesting the presence of younger, hotter stars, and perhaps ongoing star formation. Evidence of possible tidal features is weak but cannot be ruled out, given the irregularities in the light distribution. Some degree of disturbance appears present in the galaxy's overall form. It is not a perfectly smooth or regular structure.
