The galaxy appears as a somewhat flattened spheroid, exhibiting a central bulge that is significantly brighter and more concentrated than its surrounding disk. The bulge displays a yellowish hue, possibly indicative of an older stellar population. The disk component shows a mottled texture with subtle variations in color, suggesting regions of active star formation interspersed with areas of more evolved stars. There is some evidence of tidal disturbance. The galaxy has an apparent redshift, with a moderate mass estimate. It has a very low Star Formation Rate (SFR) and Specific Star Formation Rate (sSFR). It has been classified as potentially merging. 