The galaxy presents a generally smooth appearance, suggesting an elliptical or lenticular morphology. There is a slight elongation, deviating from a perfectly circular profile. Faint disturbances appear to be present within the galactic structure, possibly indicating interactions or minor mergers. The galaxy core demonstrates a concentrated brightness with a slightly bluer hue relative to its outer regions. The outer regions appear more diffuse and exhibit a slightly more greenish color. It appears no distinct spiral arms or disk-like features can be identified, lending further weight to the smooth morphological classification. The galaxy does not display obvious signs of significant merging activity, but possible remnants of an earlier minor interaction might be observable.
