The galaxy presents a generally smooth morphology, with an elliptical appearance. The light distribution indicates a relatively high concentration of older stellar populations, exhibiting a yellowish-red hue in the central bulge. There is a slight elongation observed, but no strong evidence of spiral arm structure or prominent dust lanes. The galaxy appears relatively isolated with a possible small companion galaxy nearby, that may be interacting. It is not clear if there is a merger occurring. The overall color suggests a lower rate of on-going star formation.
