The galaxy presents as an elliptical morphology, characterized by a smooth and centrally concentrated light distribution. It exhibits a relatively high degree of roundness, deviating minimally from a circular shape. The central region displays a bright, yellowish core, indicating a concentration of older stellar populations. No prominent spiral arms or distinct disk features are discernible. There is a faint, diffuse halo extending outwards from the central core, gradually fading into the background sky. There are no clear indications of ongoing major merging activity or significant tidal disturbances in the immediate vicinity of the galaxy, although some minor asymmetry cannot be entirely ruled out at this resolution. The galaxy's overall color profile suggests a relatively quiescent system with moderate to low levels of current star formation.
