The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy with a noticeable bulge. It is elongated in shape, with an aspect ratio indicating it is not a perfect sphere, possibly leaning toward a cigar shape. The central region is bright and concentrated, exhibiting a yellowish hue, which may indicate an older stellar population. There is little evidence of distinct spiral arms or significant dust lanes. The outer regions of the galaxy gradually fade into the background, suggesting a lack of ongoing, intense star formation. There might be subtle signs of tidal disturbance visible, but any recent merger activity would be either minor or very old.
