This galaxy exhibits a clear disk morphology, viewed nearly edge-on from our vantage point. The light distribution suggests a prominent central bulge, which appears smoothly distributed with a gradual transition to the disk. The dust lane appears thin and well-defined, absorbing a significant portion of the light from the disk. The overall color profile suggests a population of older stars. The disk shows no obvious signs of active star formation or spiral arm structure. There is no evidence of any major tidal disturbances or ongoing merger events. The galaxy appears relatively isolated and undisturbed.
