The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The color profile indicates a relatively old stellar population, as evidenced by its reddish hue. There is no visible dust lane or spiral arm structure. The galaxy exhibits a high degree of radial symmetry with no discernible major disturbances or tidal features, consistent with it not currently undergoing a major merger event. The galaxy appears roughly circular in shape, with no significant elongation. Although the object appears unresolved, the relatively higher concentration of light compared to neighboring objects at a similar distance indicates this is an extended object, rather than a point source. Overall, the data indicate we're observing a mature galaxy.
