The galaxy presents as a relatively smooth, elliptical object with a high degree of central concentration. Its overall shape is consistent with a spheroidal morphology. There is a bright, unresolved core, suggesting the presence of either a dense stellar population or perhaps an active galactic nucleus, though no clear indications of the latter are apparent in this image. The galaxy exhibits a color gradient, transitioning from a bluer hue near the center to a redder hue in the outer regions. This could indicate a radial variation in stellar populations, with younger, bluer stars concentrated in the core and older, redder stars dominating the outer regions. There appear to be little to no distinct spiral arm structures or prominent dust lanes visible, supporting its classification as a smooth galaxy. There are no clear signs of a major merger event, although subtle asymmetries might suggest minor interactions or past accretion events. Overall, this galaxy appears to be a well-evolved system, likely in the process of passive evolution.
