The galaxy presents as a luminous, centrally concentrated object with a generally smooth morphology. There is a noticeable elliptical structure, appearing largely round with a small deviation from a perfect circle. The central region exhibits a high surface brightness, transitioning outwards to a fainter, more diffuse halo. The color profile suggests an older stellar population, indicated by the yellowish-red hue concentrated in the center and throughout the galaxy. There is no clear indication of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, showing no signs of major merging or tidal interactions. Marginal disturbances could be occurring within, but without additional imaging it cannot be stated definitively. 
