This galaxy, at a redshift of approximately 0.328, exhibits a morphology that appears somewhat elliptical, although not perfectly spherical. It appears that most of the light is emitted from the main galactic bulge, which has a relatively smooth appearance. The minor axis is approximately half the length of the major axis, which suggests a slight elongation. There is some indication of possible tidal disturbances or interactions. I observe a faint tail-like feature extending from one side, possibly indicating a past or ongoing minor merger. A disk is also visible within the galaxy. The light from the galaxy is slightly blue-shifted, perhaps indicating active star formation. The light intensity has an absolute magnitude consistent with a fairly large galaxy.
