The galaxy appears to be an elliptical type, characterized by a smooth, diffuse light distribution. The central region exhibits a pronounced concentration of light, gradually decreasing in intensity towards the outer edges. There is no apparent spiral arm structure or significant dust lane obscuration. The overall color is yellowish, suggesting a stellar population dominated by older, redder stars. The morphology seems largely undisturbed, with no obvious signs of recent or ongoing major merger activity, and the object appears symmetrical. There are no distinct tidal features or other indicators of gravitational interaction with neighboring galaxies that are readily observable.
