The galaxy presents a morphology that is neither purely elliptical nor a well-defined spiral, exhibiting characteristics of an intermediate type. It is lenticular in shape, with a bright central bulge that appears yellowish-white, potentially indicating an older stellar population. Surrounding the bulge is a fainter, more diffuse disk component. Some asymmetry is present. One side of the disk appears slightly more extended than the other, and there seems to be a faint disturbance or tidal feature. The galaxy's light suggests ongoing, yet not vigorous, star formation activity. The colours present are consistent with a galaxy at a moderate redshift. The overall structure appears relatively undisturbed, with some subtle irregularities suggesting a past interaction.