The galaxy presents an elliptical morphology, with a smooth, centrally concentrated light profile. The core appears bright and yellowish, suggesting an older stellar population. The galaxy exhibits a faint blueish halo or extended disk, indicative of some ongoing or recent star formation, even if minimal. There is a slight asymmetry to the galaxy's overall shape. A possible tidal tail or minor disturbance is visible on the periphery. Based on the absence of strong dust lanes or spiral arms, this galaxy is likely an early-type spiral or lenticular galaxy, possibly transitioning towards a more elliptical form. Overall, the galaxy seems to be relatively isolated.
