The observed galaxy presents as a spiral galaxy, viewed at a moderate inclination. A prominent central bulge is apparent, contributing significantly to the overall luminosity of the galaxy. The bulge exhibits a relatively smooth texture, with a gradual decline in surface brightness moving outward. Two distinct, well-defined spiral arms emanate from the central region. These arms appear relatively tightly wound. There appears to be a strong central bar present. The galaxy exhibits a generally blue hue suggesting active star formation within its spiral arms. There is no apparent major mergers or disturbances.
