The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular classification. The light distribution appears centrally concentrated with a radial falloff, transitioning from a bright, yellowish core to a fainter, diffuse halo. The central region exhibits a more pronounced yellowish-orange hue, potentially indicative of an older stellar population. There is a subtle flattening of the galaxy's shape but it does not appear to be particularly elongated and can be described as round. No distinct spiral arm structures or prominent dust lanes are readily apparent. There are no obvious signs of ongoing major merger events or significant tidal disturbances, although a slight asymmetry or subtle irregularity in the outer regions might suggest past interactions or minor disturbances. Faint, extended emission surrounds the central region with a lower surface brightness. Overall, the galaxy appears relatively quiescent, consistent with a relatively low star formation rate.
