The galaxy presents as a somewhat diffuse object, exhibiting a generally elliptical morphology. The core displays a concentrated luminosity with a yellowish-white hue, suggesting a population of older stars. Moving outward from the center, the galaxy exhibits a decrease in surface brightness. The outer regions show traces of blue and green, hinting at the presence of some younger stellar populations or ionized gas, although this is not prominent. There are hints of tidal features or irregularities in the structure. These could imply a possible interaction or merger event in its past. The overall appearance suggests a galaxy undergoing some level of transition or disturbance, rather than a quiescent system.
