The galaxy presents as an elliptical morphology, elongated along its major axis, with a cigar-shaped appearance. Its light profile is centrally concentrated, exhibiting a smooth, diffuse distribution without prominent spiral arms or distinct features such as dust lanes or star-forming regions. There is a gradual decrease in luminosity from the core outwards, suggesting an absence of ongoing major mergers or tidal disturbances. The color profile appears relatively uniform with a slight reddening toward the central regions, indicative of an older stellar population. No signs of active galactic nuclei activity are readily apparent in this image.
