The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The light profile appears diffuse with a noticeable absence of spiral arm structures or a prominent disk. The color gradient suggests a relatively older stellar population, with a yellowish core transitioning to bluer hues in the outer regions. There is no evidence of ongoing major mergers or significant tidal disturbances in the immediate vicinity of the galaxy, although some minor asymmetry cannot be ruled out. The galaxy's overall roundness indicates that it is viewed close to face-on. The galaxy appears to be a spheroid. There is not a lot of ongoing star formation.
