The galaxy presents as an elliptical system, with a smooth, centrally concentrated luminosity profile. The overall shape is elongated, resembling a cigar-like appearance. The galaxy exhibits a pale blue hue, suggesting the presence of a moderate population of relatively young, hot stars. The lack of prominent spiral arms or dust lanes indicates a relatively quiescent system with low star formation activity. There are no apparent signs of major mergers or significant tidal disturbances in the immediate vicinity. However, subtle asymmetric features may suggest minor past interactions or internal dynamical processes. The galaxy appears to be a mature system with a substantial stellar mass.
