The galaxy presents as a somewhat elongated, elliptical object with a smooth, diffuse light distribution. The central region exhibits a bright, concentrated luminosity, suggesting a substantial stellar population. The overall color appears slightly redder, indicating an older stellar population and potentially lower star formation activity. There is some slight distortion evident, with the disk seeming to be slightly disturbed. There are no prominent spiral arms or dust lanes visible. The galaxy appears relatively isolated, with no obvious signs of a major ongoing merger or tidal interactions with other galaxies.
