The galaxy appears to be an elliptical galaxy, exhibiting a smooth, largely featureless morphology. It displays a concentrated central bulge, with a radial color gradient transitioning from a yellowish core to a redder outer halo. There is little evidence of spiral arms or significant dust lanes. The galaxy appears nearly circular, with a high degree of rotational symmetry. No signs of tidal tails or significant morphological distortions indicative of a recent major merger are visible. The overall color suggests a relatively old stellar population. The absence of bluer regions indicates a low rate of on-going star formation. The galaxy is unresolved, and a quantitative description of its structure requires detailed surface photometry.
