The galaxy presents as a relatively small, well-defined object with a smooth, elliptical morphology. The light distribution appears centrally concentrated, showing a gradual decrease in brightness from the core outwards, indicating a significant bulge component. There is little discernible evidence of spiral arms or a prominent disk structure. The object appears to be generally yellowish-white in color, suggesting a population of older stars. There may be some very small areas of bluer light, perhaps indicating very small regions of more recent, modest star formation. No significant distortions or tidal features are obvious, suggesting the absence of any recent major mergers or strong gravitational interactions. There may be some minor disturbances internally.
