The galaxy appears to be a relatively smooth, elliptical or lenticular type, exhibiting a centrally concentrated luminosity profile with a gradual falloff towards its outer regions. The core displays a bright, yellowish hue, suggesting an older stellar population dominating this region. Moving outwards, the color transitions slightly towards a redder shade, potentially indicative of a population shift or differential extinction. There are no prominent spiral arm structures or significant dust lanes visible, reinforcing its classification as a non-spiral galaxy. The galaxy presents a generally rounded morphology, with only a slight elongation. No signs of major mergers or tidal disturbances are readily apparent, although subtle features might be present upon closer inspection. The overall appearance suggests a galaxy that is well-evolved and relatively quiescent in terms of star formation activity.
