The galaxy presents as a single, relatively smooth structure with a concentrated central bulge that graduates smoothly outwards. The central region exhibits a yellowish-white hue, indicating a potentially older stellar population. Surrounding the core, a broader, less intense, greenish halo extends. This halo may be indicative of ongoing, but not extremely intense, star formation or a distribution of ionized gas. The overall shape approximates an ellipse with a high degree of symmetry. There is no strong indication of spiral arm structure or significant tidal disturbances; however, some subtle irregularities can be noted in the outer regions, though they could also be artifacts. The galaxy does not appear to be undergoing a major merging event, but the slight asymmetry may hint at minor interaction.
