This galaxy presents as an elongated, disk-like structure viewed nearly edge-on. The central bulge appears bright and relatively smooth, exhibiting a yellowish-white color indicative of an older stellar population. The disk is subtly visible, displaying a bluer hue compared to the bulge, suggesting the presence of younger, hotter stars and ongoing star formation, although not at a particularly vigorous rate. There is no distinct spiral arm structure readily apparent in the image. The galaxy shows no signs of major tidal disturbances or ongoing mergers, appearing relatively undisturbed and isolated. Its overall morphology points towards a late-type spiral or lenticular galaxy.
