The galaxy presents as a relatively smooth, centrally concentrated object. The overall shape is elliptical, appearing elongated but not extremely so, with the major axis oriented roughly horizontally in the image. The core exhibits a high surface brightness, appearing nearly unresolved and bright white, suggesting a significant population of older stars. The light gradually decreases with increasing distance from the center. Faint bluish hues are subtly distributed throughout the galaxy, more prominent in the outer regions, hinting at a low level of recent star formation within its disk. There appears to be no prominent spiral structure or bar. We see no signs of any major ongoing merger events or significant tidal disruption, though some small irregular features may be present.
