The galaxy presents as a disk-like structure, exhibiting a moderate inclination relative to the observer's line of sight. A prominent central bulge is visible, demonstrating a concentrated luminosity. The bulge appears to be yellowish-white in color, suggesting an older stellar population dominating this region. The disk surrounding the bulge is less luminous and appears slightly bluer, potentially indicative of younger, hotter stars and some ongoing star formation. However, distinct spiral arm structures are not clearly resolved within the disk, giving it a somewhat smooth or featureless appearance. There is no obvious evidence of a major ongoing merger event, although subtle asymmetries or minor disturbances cannot be entirely ruled out based on this image alone. The galaxy's overall morphology suggests it may be an intermediate spiral type or possibly a lenticular galaxy with a relatively faint disk component.
