The galaxy presents as a concentrated central bulge or core exhibiting a yellowish-orange hue, suggestive of an older stellar population. Fainter, diffuse extensions are noted, displaying subtle color variations, possibly indicating regions of ongoing star formation. These regions appear more reddish in some areas. The overall morphology leans towards elliptical or lenticular, with a smooth appearance. There is no clear evidence of spiral arms. The object exhibits a slightly elongated form. There might be a minor interaction or disturbance within the galaxy as there appears to be some distortion in its overall shape. 
