The galaxy presents as a single, dominant light source, with an apparent smooth morphology. The main body exhibits a concentrated luminosity, suggesting a spheroidal shape viewed near face-on. Emanating from this central region is a faint, elongated extension. This feature displays a diffuse, blue-ish tint, indicative of a possible tidal tail or disrupted arm of the galaxy. There is a lack of distinct spiral arm structures or prominent dust lanes visible within the galaxy itself. The overall color of the primary light source is redder, implying an older stellar population within the galaxy.
