The galaxy presents as a generally smooth, elliptical morphology. It exhibits a concentrated central bulge region, with a decreasing surface brightness extending outwards. There may be a faint hint of a disk-like structure although this is not immediately apparent. The color distribution suggests a population of older stars.

It has a slightly elongated shape, tending towards a cigar-like appearance rather than perfectly circular. There is no evidence of any major merger events. The galaxy does not appear to have any signs of strong recent or ongoing star formation activity. 
