The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated light profile with a high degree of central luminosity. Its shape appears to be elongated, with an axis ratio significantly less than one. The major axis of the galaxy is oriented roughly northeast to southwest.  Color gradients suggest a redder core, indicative of an older stellar population, with bluer, slightly more diffuse outer regions that may indicate lower levels of ongoing star formation. There are no immediately discernible spiral arms or prominent dust lanes. There are no major distortions or tidal features visible in the immediate vicinity of the galaxy, which indicates that it is most likely an isolated galaxy.
