The galaxy presents as a lenticular or early-type spiral galaxy, exhibiting a prominent bulge region that appears relatively smooth and concentrated. The bulge exhibits a yellowish-white color indicative of an older stellar population. A faint disk component is visible, appearing significantly flattened, with the major axis extending noticeably further than the minor axis. This disk lacks distinct spiral arm structures in this image. The color gradient suggests the disk is bluer than the bulge, implying the presence of some younger stars and possibly ongoing, but subdued, star formation. Overall, the galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or strong tidal interactions. The light distribution decreases smoothly from the central bulge outwards, with the outer regions of the galaxy being fainter and less defined.
