The galaxy presents as a relatively compact, lenticular system exhibiting a dominant central bulge. The core appears bright and concentrated, suggesting a significant population of older stars. The surrounding disk is faint, but visible, indicating a flattened structure. There are subtle hints of spiral arm structures, though they are not well-defined and appear tightly wound. Overall, the galaxy's morphology suggests a transition between a spiral and an elliptical galaxy, leaning more towards a smooth, featureless profile. A faint blue hue is present within the disk, particularly on one side, hinting at ongoing star formation. The galaxy doesn't appear to be undergoing any major merging events, however, there is a slight asymmetry to the disk, indicating a potential minor disturbance.
