The galaxy presents as a relatively smooth, elliptical object. Its color profile exhibits a dominant yellow-red hue in the central region, suggesting an older stellar population with a lower rate of ongoing star formation. The overall shape is noticeably elongated, but not strongly so. There is no distinct evidence of spiral arm structure or significant dust lanes. The galaxy appears mostly undisturbed, without any obvious signs of recent major mergers or strong tidal interactions. A very slight asymmetry can be noticed, although this could be due to image quality or subtle internal processes.
