The galaxy presents as a relatively smooth, elongated structure with a noticeable central bulge. The color distribution suggests a higher concentration of older stars in the central region, indicated by the reddish hue. Fainter, greenish tinges appear in the outer regions, suggesting the presence of younger stars and possibly ongoing, albeit low-level, star formation. The lack of distinct spiral arms or other prominent features suggests that this galaxy is likely an elliptical or lenticular galaxy. There is a slight deviation from perfect ellipticity, possibly indicating a minor interaction or disturbance in its past.
