The galaxy presents as a somewhat elongated, but mostly smooth, luminous object. The central region is significantly brighter and exhibits a yellowish-white hue, suggesting an older stellar population is dominant. The outer regions are less defined and fainter, with a slight bluish tinge on one end indicating the possible presence of younger, hotter stars or a more active region of star formation there. There's no clear evidence of spiral arms or a distinct disk. The morphology is generally consistent with an elliptical or lenticular galaxy undergoing little active star formation. There appears to be minimal tidal disturbance or interaction with other galaxies present.
