The galaxy presents as a largely featureless elliptical type, appearing smooth and diffuse. There is a concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. The outer regions transition to a slightly bluer color, indicative of some ongoing, albeit weak, star formation, although this activity seems subdued. The galaxy's shape is generally round, with only a slight deviation towards an elongated form. There is no visually apparent indication of any major disturbances or ongoing mergers. Based on the observed characteristics, the galaxy appears to be a relatively evolved system, likely nearing the end of its star-forming period.
