The galaxy presents as a relatively smooth, elliptical form, exhibiting a centrally concentrated light profile. The core region shows a bright, possibly older stellar population, indicated by its slightly redder hue. Moving outward from the center, a transition to bluer colors is observed, suggesting the presence of younger, star-forming regions.

The overall shape is elongated, deviating slightly from a perfectly circular profile. There is no clear evidence of distinct spiral arms or a well-defined disk structure. Faint irregularities may be present in the outer regions of the galaxy, possibly indicative of minor interactions or past merger events, however, further examination would be needed to say definitively. Star formation appears to be very low in the galaxy.
