The galaxy presents an overall smooth morphology, with a slight elongation suggestive of an intermediate spheroidal shape, falling between round and cigar-shaped. Its core exhibits a concentrated, yellowish hue, implying a population of older stars. The galaxy's light distribution is fairly even, with a gradual decrease in brightness from the center towards the edges. There is no apparent disk component or spiral arm structure. The galaxy doesn't seem to be undergoing any major merging activity, but slight irregularities might suggest a minor disturbance or interaction in its past, and may be in the process of quenching star formation. It displays colors of around 18-20 magnitude in the g,r, and z bands.
