The galaxy presents a somewhat elliptical morphology, appearing mostly smooth in overall structure. It exhibits a concentrated central bulge region with a yellow hue, suggesting an older stellar population. Fainter, bluer extensions emanate from the core, hinting at regions of more recent, albeit low, star formation activity. The galaxy appears to have a relatively regular form, with only slight deviations from perfect ellipticity. There is no strong evidence of ongoing major merger activity, but some minor disturbances or tidal features may be present in the faint outer regions. Overall, the galaxy appears to be a relatively massive system with characteristics of both elliptical and spiral galaxies.
