The galaxy appears as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. The light distribution suggests a dominant bulge component, with a gradual decrease in surface brightness extending outwards from the core. There is no clear evidence of spiral arms or a prominent disk structure. The color profile shows a redder core, possibly indicating an older stellar population, with a bluer halo which may indicate younger stars in the outer regions. There is no obvious sign of active galactic nucleus activity. The galaxy does not appear to be undergoing any major merger events or strong tidal interactions.
