The galaxy presents as a somewhat face-on spiral, with a discernible but not sharply defined disk structure. While there are hints of spiral arms, they are not prominent or tightly wound. The central bulge appears moderate in size and brightness, with a yellowish-white hue suggesting an older stellar population. There is a gradual fading of the light intensity from the bulge outwards into the disk, with bluer tones observed in the outer regions, indicative of younger, hotter stars and ongoing star formation. There is no obvious presence of a strong bar feature. The galaxy does not appear to be undergoing any major merging activity, though there might be some minor distortions in the outer disk which could be related to past interactions. The overall morphology suggests a galaxy in a relatively settled state of evolution.
