The galaxy presents as a relatively small, elongated object. It exhibits a somewhat smooth morphology, with a central bulge that appears moderately prominent. There are some suggestions of disk-like features, but they are not sharply defined. The galaxy's color profile indicates the presence of both older stellar populations and some recent star formation, primarily concentrated in the disk region. No significant merging activity or major disturbances are apparent within this image. The galaxy appears to be generally isolated.
