The galaxy presents as a relatively faint, disk-shaped system oriented approximately edge-on. The central bulge appears prominent and exhibits a smooth, concentrated luminosity profile, with a yellowish-white hue suggesting an older stellar population. Extending from the central bulge, a faint, diffuse disk is observed. This disk displays subtle hints of bluer light, potentially indicating regions of more recent or ongoing star formation, though the resolution limits a detailed analysis of individual star-forming regions. The galaxy's overall structure appears largely undisturbed, with no obvious signs of major mergers or significant tidal interactions. However, a slight asymmetry in the disk’s outer regions may suggest minor gravitational disturbances or ongoing accretion events. Dust lanes are not clearly apparent, but the subtle color variations across the disk could indicate the presence of patchy dust obscuration.
