The galaxy presents as a somewhat diffuse object, exhibiting a central bulge that appears relatively smooth and concentrated. The overall form is neither distinctly spiral nor elliptical, suggesting a possible intermediate classification or perhaps a galaxy undergoing a morphological transformation. A subtle extension or feature emanates from the main body which could be indicative of tidal interactions or recent merger activity, however the feature is relatively small. The color profile suggests a evolved stellar population and moderate recent star formation within the galaxy. There is a possibility the galaxy is undergoing a minor interaction or merging event which seems to be supported by the slight asymmetry in the disk structure.
