The galaxy presents as an elliptical or lenticular system, appearing smooth and relatively featureless. The galaxy exhibits a pronounced central bulge, with a high concentration of light, suggesting a significant population of older stars. There is a subtle color gradient, trending towards redder hues in the galactic core and a slightly bluer color in the outer regions. This may be indicative of some on-going, but limited, star formation within the extended galactic disk or envelope. There is no indication of a strong bar or spiral arm structure. The overall morphology is generally undisturbed, lacking evidence of significant tidal interactions or recent major mergers. There may be subtle irregularities in the outer light distribution, which could indicate minor past interactions. The galaxy is moderately distant, with a notable redshift.
