The galaxy appears as a centrally concentrated object with a generally smooth morphology. The central region exhibits a yellowish hue, possibly indicative of an older stellar population. Surrounding this core is a bluer, less defined halo. The galaxy exhibits an elliptical shape, with a noticeable extension along one axis. There is little evidence of spiral arm structure or significant dust lanes. Faint features suggest a possible minor disturbance, but the overall structure does not suggest an ongoing major merger event. The size of the galaxy appears moderate, as does the star formation rate. Overall, the galaxy presents itself as a relatively evolved system.
