The galaxy presents as a somewhat elongated, luminous structure. The light distribution appears relatively smooth, with a brighter central region that fades gradually outwards. There is a hint of asymmetry in the overall shape, possibly indicating some form of interaction or internal disturbance. The dominant color is yellowish-white, suggesting an older stellar population, although the bluer fringes imply the presence of some younger, hotter stars. The galaxy is neither perfectly elliptical nor a well-defined spiral; rather, it exhibits characteristics of an intermediate morphological type. There are no prominent dust lanes or distinct spiral arms visible.
