The galaxy presents as an object with moderate, but not perfectly smooth features. The overall form is neither definitively elliptical nor spiral. The core region exhibits a concentrated luminosity with a yellowish hue, suggestive of an older stellar population. Extending outward, the galaxy displays disrupted or asymmetric arms, possibly indicative of gravitational interactions or ongoing merger activity. Patchy regions of bluer light are present, hinting at pockets of recent star formation. There are signs of potential tidal tails or disrupted morphology, further supporting evidence of past or current interaction. The general distribution of light suggests an object experiencing significant perturbation from its initial state.
