The galaxy presents as a singular, relatively smooth and undisturbed object. The morphology appears elliptical or lenticular, displaying a generally rounded shape. There may be a slight elongation, but it is not highly pronounced. The galaxy exhibits a central concentration of light that fades gradually outwards, suggestive of an older stellar population. There's a lack of distinct spiral arms or prominent dust lanes. Based on the color profile, the light emitted is redder in hue, potentially indicating a population of older stars. There's little evidence of ongoing, widespread star formation; however, the hint of blue color could indicate a population of young hot stars. Overall, the galaxy gives the impression of being a fairly mature, relatively quiescent system.
