The observed galaxy presents a smooth, elongated morphology, suggestive of a lenticular or possibly an edge-on spiral galaxy. The light distribution appears relatively uniform, with a concentration towards the center, implying a prominent bulge. There is a slight blue tinge on the edges and possibly a faint indication of a disk structure. There are no readily apparent spiral arms or dust lanes visible, indicating a relatively quiescent star formation rate. There are no signs of major mergers or tidal disturbances. It is difficult to gauge the ellipticity precisely, however, it appears cigar-shaped. Overall, the galaxy exhibits characteristics of a relatively evolved system, likely with an older stellar population.
