The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. Its color profile exhibits a strong red-yellow hue, indicative of a population of older stars and a suppressed rate of star formation. The galaxy appears relatively isolated, though a smaller object is visible within close proximity, the object is difficult to discern from this image. The galaxy lacks any obvious spiral arm structure or dust lanes. The smooth appearance suggests the galaxy has undergone significant merging activity in the past, contributing to the homogenization of its stellar populations and morphological features. There is no evidence of current major merging or tidal disturbances; any merger event occurred in the distant past, or any ongoing mergers are too small to be visible from this perspective.
