The galaxy presents as a largely smooth, elliptical structure. It exhibits a dominant central bulge region, which appears nearly spherical in shape. The color of the central bulge is predominantly reddish-orange, suggestive of an older stellar population. A faint, disk-like structure surrounds the central bulge, displaying a greenish hue that could indicate the presence of younger stars or ongoing star formation, although the low resolution makes it difficult to confirm. The galaxy does not show any prominent spiral arms or bar features. There is some evidence of minor disturbance in the galaxy's overall structure, which could be the result of a past minor merger event. The absence of significant tidal tails or other strong signs of interaction suggests that any past merger was likely a minor event and occurred in the distant past.
