The galaxy presents a generally smooth morphology, exhibiting a notable lack of distinct spiral arms or prominent features. Its overall shape appears elongated, approaching a cigar-like appearance with a somewhat flattened profile. Color gradients are subtle, with a central region displaying a slightly bluer hue, possibly indicating a concentration of younger stellar populations or ongoing star formation activity, though at a low rate. The outer regions appear redder, potentially signifying older stellar populations. There is a subtle indication of minor disturbances present, although any evidence of ongoing or recent merging events appears weak. The galaxy's shape has some similarities to a disk, but the overall smoothness suggests more similarities to an elliptical galaxy.
