The galaxy exhibits a largely smooth morphology, appearing as a diffuse and centrally concentrated structure. There is evidence of slight elongation, suggesting a possible oblate spheroid shape, although the object does not present a disk. The dominant color is a muted orange-red hue, with what looks like a small amount of blue sprinkled in, indicating a stellar population with a relatively suppressed rate of on-going star formation. There are no obvious spiral arms or strong morphological features that might indicate recent interactions or mergers, although there is very slight asymmetry visible in the light distribution. Overall, the galaxy seems to be a mature system with a relatively high degree of internal order.