The galaxy appears as a relatively smooth, elliptical-shaped object. It exhibits a strong central bulge, with the light intensity decreasing gradually towards the outer regions. The color profile suggests a population of older stars, as evidenced by the yellowish hue. There are no prominent spiral arm structures or distinct dust lanes visible. The overall structure appears largely undisturbed, with no obvious signs of a major ongoing merger or tidal interactions. However, some slight asymmetry may indicate a minor gravitational disturbance or previous interaction.
