The galaxy presents as a lenticular or possibly a spiral galaxy, viewed at a near edge-on inclination. A prominent bulge appears centrally located, exhibiting a smooth, concentrated distribution of light, likely indicative of an older stellar population. The disk component is visually discernible but relatively faint, displaying a bluer hue suggestive of ongoing, albeit suppressed, star formation activity. No distinct spiral arms are apparent. The galaxy appears generally undisturbed, with no obvious signs of tidal interactions or recent major mergers. The overall morphology suggests a relatively evolved system transitioning away from active star formation.
