The galaxy presents as a lenticular or early-type spiral morphology, with a dominant central bulge region. The bulge exhibits a smooth, relatively featureless appearance in the available imagery, with a color profile tending toward warmer hues, suggestive of an older stellar population. There is a faint disk-like structure that has a slight reddish tint. The absence of prominent spiral arms and distinct dust lanes further supports this classification, indicating either a lack of significant recent star formation or a viewing angle that obscures such features. The galaxy's overall shape appears elongated, hinting at a possible elliptical form, but this may be due to an edge-on perspective of the disk component. There appears to be little evidence of ongoing mergers or major tidal interactions.
