The galaxy appears to be an elliptical type, exhibiting a generally smooth morphology without prominent spiral arms or a distinct disk structure. The light distribution suggests it is moderately concentrated. There is a somewhat elongated shape, though not highly cigar-shaped. The color profile indicates a redder central region, transitioning to a slightly bluer, more extended halo. The red color is possibly indicative of an older stellar population, while the slight bluer components suggest the presence of some younger stars. Based on the irregularity of the shape, it is potentially undergoing a merger or has experienced one recently, as there appears to be some gravitational disturbance to its structure. The presence of a merging signature would be considered minor rather than major.
