The galaxy presents as a somewhat diffuse, elliptical structure. The core region is noticeably brighter, exhibiting a concentrated luminosity gradient. The overall color appears to be bluish-white, hinting at the presence of a younger stellar population, albeit subtly. There is a slight elongation to the galaxy's shape, classifying it as an elliptical type closer to being in between round and cigar shaped than either of those individual types. No distinct spiral arms or prominent dust lanes are discernible. The galaxy appears relatively isolated with no obvious signs of interaction with nearby galaxies in this particular field.
