The galaxy presents as a relatively well-defined spiral, observed at an angle neither directly face-on nor edge-on. There is evidence of spiral arm structure, although somewhat flocculent and not sharply delineated. The central bulge appears moderate in size, exhibiting a yellowish hue suggestive of an older stellar population. A bar-like structure may be present, though not prominently featured. The disk shows a bluer color than the bulge, indicative of ongoing star formation. Overall, the galaxy does not show signs of major mergers or significant disturbances, though some degree of interaction or minor tidal features might be present. The galaxy exhibits characteristics of intermediate-mass spiral galaxies with moderate levels of star formation.
