This galaxy exhibits a generally smooth morphology with a slight central bulge. The light distribution suggests a dominant spheroidal component. There is evidence of a faint disk structure, with a high likelihood of the disk being viewed edge-on. The disk appears relatively featureless, lacking prominent spiral arms or distinct dust lanes. Overall color is relatively uniform throughout, tending towards the red end of the spectrum. No prominent ongoing mergers or major disturbances are visible. However, it cannot be ruled out that some disturbance is happening on a smaller scale. Star formation rates appear quite low. The galaxy is estimated to be of intermediate mass.
