The galaxy presents as a moderately elliptical system. The core is bright and concentrated, indicating a possible bulge. The overall light distribution appears smooth, with no distinct spiral arm features visible. The galaxy's colouration shifts from a bluer hue in the central region to redder tones toward the outer edges, suggestive of an older stellar population dominating the periphery. No signs of significant tidal disturbances or merging events are evident. The axial ratio indicates that the galaxy is not perfectly spherical but exhibits a noticeable ellipticity, resembling an E4 classification, or maybe even higher.
