The galaxy exhibits a primarily smooth morphology, with a slight preference towards an intermediate elliptical shape. The central region displays a yellowish-orange hue, indicative of an older stellar population. This core is surrounded by a less concentrated, bluer halo, suggesting the presence of some younger stars and ongoing star formation activity, though at a modest rate. No distinct spiral arm structures are visible, nor are there any obvious signs of major tidal disruption or recent merger events. Minor irregularities may be present in the outer regions, potentially hinting at minor interactions. Overall, the galaxy appears to be a relatively undisturbed system transitioning between a spiral and an elliptical galaxy.
