This galaxy presents as an elongated, lenticular structure, with an apparent blue shift along its major axis, suggesting possible rotational dynamics. The galaxy exhibits a relatively smooth texture throughout its primary body with a slight concentration in the center. A faint tail-like structure extends from one end of the galaxy, possibly indicative of tidal interactions or ram-pressure stripping from the intergalactic medium. This tail exhibits enhanced green color, which might correlate with increased presence of certain emission lines. Based on the object's apparent color and morphology, the galaxy likely has a mass between 10^9 and 10^10 solar masses, and a size of about 6 kpc, with a relatively low star formation rate. There is a relatively high probability that it is not undergoing any major mergers.
