The galaxy presents as a somewhat elliptical, centrally concentrated structure. The core exhibits a bright, yellowish hue, suggestive of an older stellar population. Fainter, bluer extensions appear on either side of the core, possibly indicating regions of more recent star formation, though these features lack well-defined spiral arms. There is a slight asymmetry, with one side appearing slightly more extended. The overall impression is of a system transitioning from a more active star-forming phase to a more quiescent, redder state. There are hints of a possible minor tidal disturbance, but a merger event is not clearly indicated.
