The galaxy presents as an elliptical type, appearing mostly smooth and relatively featureless. Its shape is more akin to an intermediate ellipse, deviating mildly from being perfectly circular, but not notably elongated either. The core region exhibits a bright, concentrated luminosity, suggestive of a high stellar density or potentially an active galactic nucleus. A subtle color gradient is present, with the central regions exhibiting a slightly yellow hue, potentially indicative of an older stellar population. The outer regions show a slight shift towards bluer tones, which may signify the presence of younger, hotter stars, perhaps due to minor ongoing star formation, though at a low rate. There is no obvious indication of ongoing major merging activity, tidal tails, or other significant disturbances in the galactic structure, but a faint, small disruption is visible on one side of the galaxy. The light is redshifted, so it is approximately 3.2 kiloparsecs in size.
