The galaxy presents as a largely smooth, elliptical-like structure, exhibiting a high degree of central concentration of light. The overall color profile suggests a dominant population of older stars, with a gradual shift towards redder wavelengths from the core outwards. There is a subtle indication of a disk feature to the upper-left and a faint tail feature to the lower-right of the galaxy, suggestive of a possible minor disturbance or past interaction. However, these features are not pronounced, and the galaxy appears largely undisturbed. The shape of the galaxy is more round than cigar-shaped. 
