This galaxy exhibits a morphology suggestive of a system undergoing a merger or interaction. The light profile is not smooth; instead, it shows a disturbed structure with multiple luminous cores or clumps distributed along a somewhat linear axis. The dominant color is yellow, indicating a substantial population of older stars, although some areas show slightly redder hues, possibly indicative of either dust obscuration or a population of redder stars. The presence of multiple cores and the disrupted light distribution points toward a dynamic process affecting the galaxy's structure, very likely a galaxy merger. The galaxy presents a moderate amount of star formation, with a mass log of approximately 11.4. The overall shape is neither perfectly elliptical nor a clear spiral, hinting at a transitional phase in its evolution influenced by the gravitational interactions.
