The galaxy presents as a relatively smooth, rounded structure, exhibiting a dominant elliptical morphology. There is an absence of clear spiral arm features. The light profile appears largely uniform across the galaxy's body, with a concentration towards the center.

The galaxy displays a redder color, suggesting a population of older stars and a subdued rate of star formation. No evidence of ongoing major mergers or significant tidal disturbances is observed. The galaxy appears relatively isolated and undisturbed in this particular field of view.
