The galaxy presents as a relatively smooth, elliptical structure. It is somewhat elongated, exhibiting a cigar-like shape. The galaxy's core region displays a brighter, more concentrated luminosity, indicating a dense stellar population or potentially an active galactic nucleus. The surrounding halo appears less defined, with a gradual decrease in brightness outward. There is no apparent disk structure, spiral arms, or significant dust lanes visible. There is a subtle indication of a minor disturbance in its morphology, possibly hinting at a past or ongoing minor interaction. The dominant color is a yellow-orange hue, suggesting a population of older, redder stars. Star formation appears minimal. 
