The galaxy presents as a moderately compact, lenticular or early-type spiral, displaying a generally smooth morphology. It shows a distinct ellipticity, being somewhat cigar shaped. Evidence of internal structure is subtle, with a slight suggestion of faint, tightly wound spiral arms or dust lanes, though the smooth overall appearance dominates. There is no obvious bright central bulge. No tidal features or significant disturbances indicating recent merger activity are visible. The color profile suggests an older stellar population, with a bias towards redder hues rather than the blue associated with active star formation. The galaxy is oriented approximately vertically in the image.