The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or lenticular galaxy at an approximate redshift of 0.097. The object is not perfectly circular, appearing somewhat elongated or 'in between' round and cigar shaped along its major axis. There is a subtle color gradient, with a bluer hue towards the central region and a slight reddening towards the outer regions. This subtle change could be indicative of older stellar populations dominating the outer regions of the galaxy with ongoing star formation in the center. No prominent spiral arm structures or obvious dust lanes are visible, suggesting it's a morphologically evolved system. There is no evidence of significant tidal features or ongoing major mergers, although a minor disturbance cannot be ruled out. Based on these observations, this is likely a moderately massive galaxy with a low-to-moderate star formation rate.
