The galaxy presents as an elongated, disk-like structure, likely a spiral galaxy viewed at a high inclination angle. The central bulge appears prominent, exhibiting a yellowish-orange hue, suggestive of an older stellar population. The disk shows a mottled texture, with hints of bluer regions along the edges, potentially indicating areas of more recent star formation. There may be some minor disturbances and/or interactions with other structures. Overall, the galaxy exhibits a relatively smooth morphology, but does not appear to be perfectly elliptical. The galaxy is fairly compact, and no strong signs of merger activity are visually apparent.
