The galaxy presents an elongated, cigar-shaped morphology. It exhibits a smooth, diffused appearance with a concentration of light toward the central region, suggesting a prominent bulge. The color profile indicates a reddish hue, possibly indicative of an older stellar population or significant dust obscuration. There's a hint of a faint, diffuse disk structure surrounding the bulge. The lack of discernible spiral arms or distinct features suggest the classification of an elliptical galaxy, with a high probability of little to no current major merging events. There appears to be a small object nearby, potentially a small satellite galaxy, but it is very faint and may not be gravitationally bound.
