The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The overall color gradient transitions from a yellowish-white core to a bluer halo. The galaxy displays a high degree of radial symmetry, with a slight deviation suggesting a possible minor disturbance or interaction.  There is little evidence of distinct spiral arms or significant dust lanes. The outer regions of the galaxy appear diffuse, fading into the background sky. The overall morphology suggests a relatively evolved system, potentially dominated by an older stellar population. The effective radius of the galaxy, judged by the visible extent, is approximately 5 kiloparsecs. Star formation appears to be present, but it is likely at a low rate.
