The galaxy presents a largely elliptical morphology, appearing quite smooth and lacking prominent spiral arm structures or significant dust lanes. The light distribution suggests a concentration of older stellar populations, with the core exhibiting a yellowish-orange hue. The outer regions of the galaxy fade gradually into the background sky, indicating a diffuse stellar halo. There's a very slight asymmetry to the galaxy's overall shape, but this is negligible and it can be considered to be fairly round. Based on the low level of observable star formation, this is likely a quiescent galaxy with minimal ongoing star formation. There are no signs of any major mergers or tidal disruptions. The overall appearance points towards a galaxy that is well evolved and gravitationally stable.
