The galaxy appears as a centrally concentrated, luminous object with a smooth, diffuse morphology. Its overall color is yellowish-orange, suggesting a dominant population of older stars. There is no clear evidence of spiral arm structure or prominent dust lanes. The galaxy exhibits an elliptical shape, and its light profile appears relatively uniform, gradually decreasing in intensity from the core outwards. Minor tidal disturbances cannot be ruled out, though the overall structure appears relatively undisturbed. The galaxy's estimated size is considerable, with its central region compact and well-defined. The absence of distinct blue regions or bright star-forming knots implies a low star formation rate.
