The object appears to be a lenticular or early-type spiral galaxy, displaying a flattened, disk-like structure. The central bulge is prominent and exhibits a relatively smooth, featureless appearance, suggesting an older stellar population.  The disk is oriented nearly edge-on, which obscures any spiral arm structure that may be present. There is a noticeable dust lane bisecting the galaxy along its major axis, causing significant obscuration. The galaxy exhibits a color gradient, with the central bulge appearing more yellow/orange, potentially indicating a higher concentration of older, redder stars. The outer regions are dimmer and show hints of bluer colors, possibly indicative of some ongoing, albeit low, levels of star formation. The galaxy's overall structure appears undisturbed, with no obvious signs of recent major mergers or tidal interactions.
