The galaxy presents a moderately bright profile, exhibiting a distinct morphological structure indicative of an ongoing or recent merger event. The central region appears smooth and spheroidal, contributing to approximately half of the galaxy's visual appearance, and possesses a yellowish hue, suggesting an older stellar population. Extending outwards from this central region, are discernible features indicating disruption, with faint streams of stellar material and tidal tails. The overall color gradient shifts toward redder hues, which correlates to regions with a greater concentration of older stars and potentially higher dust content. Patches of bluer color are scattered throughout the galaxy, providing evidence of ongoing or recent star formation, which does not significantly contribute to the overall color profile. A significant portion of the galaxy suggests it is a merger and is displaying signs of tidal forces at work. The object exhibits a disturbed morphology, rather than a quiescent, well-defined spiral or elliptical form.
