The galaxy presents as a single, relatively smooth and concentrated object. Its light is centrally concentrated, with a roughly circular profile. The light profile decreases gradually from the center to the edge with no defined core. The galaxy appears to be slightly more luminous in the redder bands of the visible spectrum, but still displays some blue light. There are no obvious spiral arm structures or prominent dust lanes visible. A hint of a more diffuse halo is present, but the data is insufficient to resolve any fine details within it. Overall, the galaxy presents a fairly uniform appearance, suggesting a spheroid-dominated morphology. There is no evidence of recent or ongoing major merger activity or significant tidal disturbances.
