The galaxy presents as a single, relatively smooth object with a concentrated central bulge. The light appears to be dominated by older stellar populations, exhibiting a yellowish-orange hue indicative of evolved stars. There is no strong evidence of spiral arm structure or significant dust lanes visible in this image. The galaxy appears mostly elliptical, verging on circular, with no significant tidal features or morphological disturbances suggesting recent major merger events. The apparent lack of substructure implies a relatively quiescent state. There might be very faint bluer regions in the outer extent of the galaxy indicating some younger star formation, but this is not a dominant feature of the galaxy's overall appearance.
