The galaxy presents a predominantly smooth morphology, indicating a lack of significant spiral arm structure or prominent dust lanes. The light distribution appears centrally concentrated, with a gradual decrease in intensity moving outwards. It exhibits an elliptical shape, although it does show some signs of deviation from perfect roundness. The central region of the galaxy displays a yellowish hue, potentially suggesting an older stellar population and a lower rate of ongoing star formation compared to the bluer outskirts. There are no strong indicators of recent major merger events or significant tidal disturbances in its overall structure. Minor disturbances or interactions cannot be entirely ruled out, but are not readily apparent from the image.
