This galaxy appears to be a relatively smooth, elliptical-like structure. The central region exhibits a concentrated, bright core, which likely indicates a significant population of older stars. Moving outward from the core, the luminosity gradually decreases, suggesting a decline in stellar density. There are hints of a flattened shape, possibly between round and cigar-shaped, but it is dominated by a relatively homogenous structure without obvious spiral arms or significant dust lanes. The galaxy presents a yellow-orange hue overall, consistent with a dominant population of older stars. There might be some minor disturbance, as some asymmetry seems visible. No presence of distinct tidal tails or prominent merging companions are observed.
