The galaxy presents as a relatively smooth, elliptical-like structure. Its overall shape appears to be somewhere between round and elliptical, exhibiting a slight elongation but lacking any pronounced disk features. The color profile suggests a dominant population of older stars, as indicated by the yellowish central bulge which is surrounded by a more blueish light. There is no apparent evidence of ongoing major merging activity or significant tidal disturbances in its immediate vicinity, with only minor irregularities that could potentially signify minor interactions. The galaxy shows a somewhat subdued presence of star formation.
