The galaxy presents as a single, relatively smooth object with an elliptical morphology. It exhibits a pronounced central bulge that is brighter and more concentrated than the surrounding galactic disk. The color gradient indicates an older stellar population, with a yellowish-orange hue dominating the central region. The outer regions of the galaxy display a slightly bluer tinge, suggesting the presence of some younger stars, although star formation appears to be subdued. The galaxy's overall structure is well-defined, with no obvious signs of significant tidal disturbances or ongoing major merger activity. There may be faint evidence of a disk-like structure around the bulge, but it is difficult to discern. The object appears to be an early-type galaxy with a modest level of recent star formation.
