The observed galaxy presents as an edge-on spiral or lenticular galaxy, with a noticeable bulge. The galaxy exhibits a smooth texture and elliptical shape. The color gradient suggests older stellar populations dominate, with a reddish-yellow hue concentrated in the central bulge. This implies the bulge is likely composed of older stars. The visible disk appears relatively thin and faint, which may indicate a low rate of on-going star formation or it could be obscured by dust. There is no clear evidence of recent merging events or significant tidal disturbances.