The galaxy presents as a somewhat elliptical morphology. The core appears to be luminous and concentrated, showing a smooth, bright, and almost featureless profile in the central region. Faint extensions emanate outwards, suggesting a diffuse halo or envelope surrounding the core. There is a hint of substructure or asymmetries within the outer regions of the galaxy, with suggestions of possible tidal features or minor disturbances. The galaxy appears to be moderately inclined relative to our line of sight. There is no clearly defined disk component apparent. The color distribution suggests that the galaxy is dominated by an older stellar population.
