The galaxy presents as a disturbed system, most likely undergoing a merger. Its overall shape is irregular, lacking a well-defined structure. There's evidence of tidal features, perhaps faint tails or bridges, extending outwards from the main body of the galaxy. The central region appears to be a blend of diffuse light, potentially indicating ongoing or recent star formation activity. There are concentrations of redder light suggesting a higher population of older stars, likely a central bulge. A portion of the galaxy exhibits a bluer hue, suggestive of younger, hotter stars within star-forming regions. The distribution of light within the system is uneven, with some areas appearing brighter and more concentrated than others. This unevenness may be due to the ongoing merger process, which can compress gas and dust, triggering bursts of star formation.
