The galaxy presents a generally smooth morphology with a concentrated central bulge. The color profile suggests an older stellar population, with the core exhibiting a yellowish-orange hue. A subtle disk-like structure appears to surround the bulge, though features are indistinct. It does not appear to be undergoing any major mergers or strong tidal interactions, though faint asymmetries may suggest minor gravitational disturbance. The object shows a relatively high degree of central concentration with gradual decline in surface brightness away from the core. The galaxy shows a modest level of star formation.
