The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a yellowish-orange hue, suggesting a dominant population of older stars. No distinct spiral arms or bar structures are discernible. The galaxy's light profile fades gradually from its core, indicating a lack of significant ongoing star formation. There is no apparent evidence of tidal features, major mergers, or strong gravitational interactions. The shape is round. The galaxy appears relatively isolated in this field of view.
