The galaxy presents a generally smooth and rounded morphology, appearing elliptical in shape. A bright central bulge dominates the structure, with a gradual decrease in luminosity towards the outer regions. There's a hint of asymmetry in the outer regions; it's not perfectly round. The galaxy appears to have a yellowish hue, suggesting an older stellar population and a relatively low rate of ongoing star formation. No significant dust lanes or spiral arm structures are discernible. There is no clear evidence of any major ongoing merging activity, or strong tidal disturbances in its appearance.
