The galaxy presents a largely smooth morphology, exhibiting an elliptical shape. The central bulge displays a concentrated, bright yellowish-white hue, suggesting a substantial population of older stars. Moving outward from the bulge, the light gradually diffuses into a fainter, more bluish halo. There appears to be little or no indication of prominent spiral arm structures, dust lanes, or ongoing active star formation in the visible light spectrum. The galaxy’s overall form is elongated, with the major axis exceeding the minor axis by a notable margin, although it does not have the most extreme elongation. No significant tidal disturbances or signs of recent mergers are immediately apparent in the image.