The galaxy presents as an elliptical or lenticular system, exhibiting a generally smooth and concentrated morphology. A bright central bulge is apparent, transitioning to a less defined, fainter outer region. The overall color profile suggests a population of older stars, indicated by the reddish-yellow hue dominant throughout the galaxy, especially towards the core. No prominent spiral arms or significant dust lanes are discernible. There may be some slight asymmetry in the shape. This morphology indicates the likelihood of the galaxy being relatively evolved, with a low rate of ongoing star formation.
