The galaxy presents as an elongated, disk-like structure viewed edge-on. A prominent central bulge is visible, exhibiting a yellowish-orange hue suggestive of an older stellar population and/or significant dust obscuration. The disk component appears relatively smooth, with hints of blueish diffuse light extending from either side of the central bulge. These regions likely indicate ongoing star formation. The absence of clearly defined spiral arms, coupled with its smooth appearance, suggests a potentially lenticular or relatively quiescent spiral galaxy morphology. There is a slight asymmetry in the disk's extent on either side of the bulge, possibly indicative of a minor tidal interaction or internal disturbance. Overall, the galaxy appears relatively isolated and undisturbed.
