The galaxy presents a generally smooth and elliptical morphology. It exhibits a concentrated central bulge that dominates its overall luminosity. The color profile suggests an older stellar population, particularly within the bulge, indicated by its yellowish hue. The outer regions show fainter, bluer light, which could indicate the presence of some younger stars, though at a lower overall star formation rate. There is no evidence of strong spiral arms or a well-defined disk structure; however, a subtle flattening is discernable indicating it is not perfectly circular. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There is the possibility of slight morphological distortions but they appear minor.
