The galaxy presents as a relatively smooth, flattened spheroid. A central bulge, exhibiting a yellowish hue, is evident. Extending outwards from this central region is a fainter disk component, showing a bluer color profile compared to the core. There are no easily discernible spiral arms within the disk, nor is there strong evidence of recent major merger activity or significant tidal disturbances affecting the system's overall structure. There is a slight extension or asymmetry to the left of the central region, suggesting a possible minor interaction or internal feature, but further data is needed to confirm this. Overall, the galaxy appears to be a disk galaxy with a substantial bulge and a relatively quiescent star formation history.
