The galaxy presents a largely smooth and rounded morphology, suggesting a classification towards the elliptical end of the Hubble sequence. There is little evidence of spiral arm structures or significant disk-like features. The light distribution is centrally concentrated with a relatively even gradient towards the outer edges. The galaxy exhibits a dominant yellow-orange hue, possibly indicative of an older stellar population. The colour suggests a relatively quiescent star formation rate, with a population of evolved stars contributing significantly to the observed light. There are some faint, small redder objects in the vicinity, possibly star forming areas, though the overall picture indicates that it is not a very active galaxy. There are no prominent tidal tails or obvious signs of recent major merger events. The high degree of observed smoothness implies that any past interactions have likely been well-mixed, and that the galaxy is now in a relatively relaxed state.
