The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, exhibiting an approximate aspect ratio of near 1:1, with only a slight deviation from circularity. A dominant, bright central bulge is readily apparent, appearing redder in color compared to the outer regions. The outer regions display a bluer hue, suggesting the presence of younger stellar populations or ongoing star formation in these areas, though at a low rate. There is no visible evidence of spiral arm structure or a prominent disk. There appears to be some minor morphological disturbance, though no major interactions with other galaxies seem to be present.
