The galaxy presents as a moderately luminous, relatively compact object at a redshift of approximately 0.062. It exhibits a roughly elliptical morphology, with a concentrated central bulge that appears primarily yellow, suggesting a population of older stars. There's a subtle disk-like structure extending from the bulge, which is also relatively smooth in appearance, but displays hints of blue hues that indicate the presence of younger stellar populations. The galaxy doesn't show any clear signs of major tidal disturbances or ongoing mergers, though very subtle irregularities in the outer regions cannot be entirely ruled out. Its overall mass estimate is relatively high, but its star formation rate appears to be comparably low, implying a galaxy that is likely in a transitional phase between actively star-forming and quiescent. The system displays a mixture of smooth features and potential disk components, with most observations indicating little to no merging activity.