The galaxy presents a moderately bright, primarily smooth morphology, with a slight elongation. Its color profile indicates a prominence of older stellar populations, evidenced by its redder hue. There is a subtle indication of a disk structure, but this is not a dominant feature. Faint, diffuse extensions might be present, potentially suggesting minor tidal interactions or past merger events. The central region appears more concentrated and brighter than the outer regions. Overall, the galaxy appears relatively undisturbed.
