The galaxy presents as a moderately bright, elliptical-like structure. It exhibits a concentrated central bulge that appears largely featureless and smooth, with a yellowish hue. The galaxy displays a gradual radial decline in surface brightness from the core outwards, with a subtle transition to a more diffuse halo. There's little evidence of spiral arms or prominent dust lanes. The overall morphology suggests a relatively evolved system, potentially indicative of an older stellar population.
