The galaxy presents as a smooth, elliptical object, exhibiting a significant bulge component. Its light profile suggests a centrally concentrated distribution. The light appears redder in color, indicative of an older stellar population with relatively suppressed star formation. The galaxy displays an elongated shape, with a clear major axis visually distinguishable from its minor axis. It is classified as an edge on disk. No prominent dust lanes or spiral arm structures are discernible in the image, implying that the object is likely an early-type galaxy. No merging activity is seen in this galaxy. The object lacks any distinct features suggestive of ongoing interactions. The galaxy has an estimated diameter of about 3.5 kpc.
