The galaxy presents as an approximately elliptical, disk-dominated system, observed at an oblique angle, but not perfectly edge-on.  A central bulge is evident, displaying a bright, concentrated luminosity. The disk appears to have spiral arm structures exhibiting broad features with some irregularities and patchiness throughout, suggestive of active star formation regions. The galaxy's color profile indicates a mix of stellar populations, with a general trend of bluer hues towards the outer disk, indicative of younger stars, and redder hues concentrated within the central bulge, representing a population of older stars. The overall morphology indicates a system which has likely undergone some minor gravitational interactions.
