The galaxy presents as a relatively smooth and centrally concentrated object. There is evidence of a faint, extended disk surrounding a brighter, more spheroidal central region. The overall color of the galaxy appears to be somewhat blueish, particularly in the central region, possibly suggesting the presence of younger stellar populations and ongoing star formation. The galaxy displays a slight elongation. No distinct spiral arms or prominent features such as dust lanes are readily apparent. The overall morphology is suggestive of an intermediate type galaxy between a pure elliptical and a spiral, possibly a lenticular (S0) or an early-type spiral galaxy, with a dominant bulge component. There might be some minor disturbances in its structure, potentially hinting at a past or ongoing interaction with another galaxy, but it does not appear to be a major merger.