The galaxy presents as a luminous, elliptical structure. Its overall color appears to be on the redder end of the spectrum, indicative of an older stellar population and relatively low levels of current star formation activity. The galaxy's morphology is primarily smooth, with a notable absence of distinct spiral arms or a prominent central bar. There is a slight elongation to the galaxy's shape, but it does not deviate significantly from a generally rounded form. The galaxy appears relatively isolated, showing no obvious signs of major interactions or mergers with other galaxies, though a slight asymmetry in its outer isophotes hints at a possible minor disturbance in its past. Its size is not particularly large, but it is still a substantial object. Based on these observations, the object is likely an elliptical galaxy at a moderate distance.
