The galaxy presents as a relatively smooth, elliptical object with an overall round morphology. Its light is dominated by a yellowish-white hue, suggesting an older stellar population. There is a faint indication of a slight flattening or disk-like structure, but this is not prominent. No distinct spiral arms or significant dust lanes are visible. There is no apparent active galactic nuclei or strong star formation. There are no major disturbances or signs of merging activity. The galaxy appears to be an isolated system, evolving passively.
