The galaxy presents as a moderately bright, elongated structure with a smooth, diffuse appearance. The central region exhibits a concentrated luminosity, suggesting a prominent galactic bulge. The overall color profile leans towards the redder end of the spectrum, particularly in the central bulge, transitioning to slightly bluer hues in the outer regions of the disk. There are no clear spiral arm structures visible, indicating a relatively featureless disk. The ellipticity of the galaxy is noticeable, suggesting that it is not viewed face-on. There is no apparent interaction with neighboring galaxies or signs of ongoing major merger activity, though subtle disturbances cannot be ruled out. The overall morphology appears to be consistent with that of an early-type spiral or lenticular galaxy, with a relatively passive star formation rate.
