The galaxy presents a primarily smooth morphology, with a slight elongation suggesting a possible elliptical form, though it is somewhat in between round and elongated. There is very little apparent substructure or distinctive features, and no clear evidence of spiral arms or a bar. A merging event may have been observed in the past, indicated by minor disturbances in the galaxys shape. The color profile shows a concentration of light within the central region. The overall color appears to be a moderate yellow which suggests an older stellar population, with low star formation activity. The galaxy appears to be a substantial galaxy, with estimates of its size placing it in the medium range for galaxies in the observed sample.
