The galaxy appears to be undergoing a significant merger event. Two distinct luminous cores are visible, suggesting the presence of two interacting galaxies. The overall morphology is highly disturbed, lacking a clear spiral or elliptical structure. A faint, diffuse halo surrounds the brighter central regions. The color profile suggests the presence of a significant population of older stars, with the overall hue trending toward redder wavelengths. There might be some tidal features, but low resolution prevents definitive confirmation. The interaction appears to be in a relatively advanced stage, as the cores are in close proximity. The luminosity distribution across the galaxy is uneven, with the central regions exhibiting significantly higher surface brightness compared to the outer regions. There is a slight asymmetry in the outer regions, suggesting potential ongoing tidal interactions.
