The galaxy presents as a generally smooth and centrally concentrated object. It exhibits a moderately elliptical shape, appearing more oblong than perfectly circular. The central region is bright, suggesting a concentration of stars, possibly indicative of a bulge. The light gradually diminishes from the center outwards. Faint hints of spiral structure are not ruled out, however they are ill defined. There is no clear evidence of significant tidal disturbances or ongoing major mergers with other galaxies. The galaxy exhibits a relatively red color, consistent with a population of older stars and a low rate of current star formation.
