The galaxy presents an elliptical morphology, displaying a smooth, featureless light distribution. The luminosity profile is centrally concentrated, peaking at a bright, yellowish core. There is a gradual decrease in surface brightness moving outwards from the core, forming a diffuse halo. The galaxy appears slightly elongated, exhibiting a moderate axial ratio. No prominent spiral arms, dust lanes, or star-forming regions are readily discernible in this image. The overall color is moderately blue-white, indicating the presence of a significant population of intermediate-age stars. Minor disturbances might be present in the outer halo of the galaxy, possibly indicative of past minor merger events or tidal interactions. The galaxy appears relatively isolated, with no nearby interacting galaxies evident in this field of view.
