This appears to be an edge-on spiral galaxy. The primary axis is elongated and vertically oriented. A bright, centrally concentrated bulge dominates the visual appearance. The disk component is characterized by a relatively smooth texture, with a faint blue hue, suggestive of ongoing or recent star formation. There is also a slight hint of dust lane absorption along the midplane of the galaxy, further supporting the classification of a spiral galaxy. The lack of obvious spiral arms indicates the galaxy is likely a late-type spiral or a lenticular galaxy viewed edge-on. There are no readily apparent signs of significant tidal interactions or major mergers, although slight asymmetries are observed suggesting minor disturbances may be present. The bulge appears to be boxy or peanut-shaped, implying past bar-induced morphological transformations.
