The galaxy presents as a single, relatively smooth structure with a concentrated central region. There is an elliptical morphology, tending toward a spheroidal shape rather than a well-defined disk. The light distribution exhibits a radial gradient with a bright, yellowish core that diminishes gradually outwards into a bluer, less luminous halo. There is no clear indication of spiral arms or strong dust lanes. Subtle irregularities in the outer regions could suggest minor disturbances, but the overall impression is one of a settled system, possibly an early-type galaxy, with a relatively low star formation rate. The galaxy appears to be moderately massive, considering the overall light output and physical size.
