The galaxy exhibits a generally smooth morphology, with a dominant, centrally concentrated component exhibiting a distinct blue hue. This core appears largely spheroidal, with a moderate degree of roundness. Fainter, less defined, features of a yellower color, extending outward from the core, suggest the possibility of a disrupted disk or tidal tails, indicating a potential interaction or merger event in the galaxy's past. There is no strong evidence of active star formation in the central region. These observations are consistent with a galaxy that has undergone, or is undergoing, a merger, with a significant population of older stars dominating the overall light profile. The estimated size is relatively compact, implying that any interaction may be in its earlier stages.
