The galaxy appears as a moderately bright, elliptical-shaped object. Its central region exhibits a yellowish-white hue, suggesting an older stellar population and low star formation activity. The outer regions display a subtle gradient, fading into a bluish tint, potentially indicating the presence of younger, hotter stars. The overall smoothness of the light distribution suggests a lack of significant spiral arm structure or prominent dust lanes. The galaxy seems relatively undisturbed, without any obvious signs of recent major mergers or tidal interactions. The shape is elongated, not quite circular, with an axial ratio suggesting a classification between E4 and E6 on the Hubble sequence. There may be some evidence of minor disturbances in the outer halo of the galaxy, but more data is required to confirm.
