The galaxy presents as a single, largely featureless object with a smooth morphology. It appears approximately round, exhibiting a high degree of radial symmetry. The galaxy's color is notably yellowish-orange, suggesting a relatively older stellar population with diminished recent star formation. There is a faint, gradual decline in brightness from the core outwards, consistent with the light distribution of an elliptical galaxy. No distinct spiral arms, bars, or dust lanes are visible. There appears to be no evidence of significant tidal disturbances or ongoing mergers. The galaxy appears to be relatively isolated, without obvious companions or signs of interaction in its immediate vicinity.