The galaxy presents as a centrally concentrated object, exhibiting a generally elliptical morphology with a fuzzy, ill-defined edge. There is evidence of a central bulge which appears slightly more yellow/red than the rest of the disk, potentially indicating an older stellar population. The overall color is indicative of a relatively mature system, although some bluer regions are apparent, particularly surrounding some of the redder areas. These likely indicate regions of younger star formation. There are some disturbances, such as minor disruptions in the galaxy shape and color which suggests a recent or ongoing minor merger event. The inner region of the galaxy shows some potential signs of disturbance as well, which may be related to tidal effects from a previous interaction. There are some indications of asymmetry in the color distribution, with the west side possibly having more red color.