The galaxy presents as a somewhat smooth, centrally concentrated object. Its overall morphology appears elliptical or lenticular given the lack of prominent spiral arm structure. The central region exhibits a yellowish hue, suggesting a higher concentration of older stellar populations. Moving outward from the core, there is a subtle decrease in the concentration of light, with a transition toward slightly bluer tones in the outer regions, indicating the potential presence of some younger stars or star-forming regions. There is no obvious sign of a major ongoing merger. The is a hint of some distortion nearby, indicating a possible minor interaction with another smaller galaxy or gas cloud.
