The galaxy presents as an elliptical morphology. The central region exhibits a concentrated, bright core with a yellowish-orange hue, suggesting an older stellar population. Surrounding this core is a fainter, more diffuse halo with a slightly greenish tint, which could indicate the presence of some younger stars or ionized gas, although it's not particularly prominent. The overall structure appears smooth, with no discernible spiral arms or significant dust lanes. The galaxy has a fairly round shape, with only a slight elongation. There is no apparent evidence of major mergers or significant tidal disturbances.
