This galaxy exhibits a primarily smooth morphology, with a centrally concentrated light profile suggesting an elliptical classification. It appears nearly round, with a slight deviation toward an intermediate shape rather than a highly elongated or cigar-shaped form. The galaxy displays a dominant yellowish-orange hue in its central region, which could indicate an older stellar population. There is very little evidence of spiral arm structure or prominent dust lanes. Based on the image, there is little sign of major or minor disturbances to the galaxy's overall structure, or of an active merger event, with the majority of classifications suggesting no merger is present. The galaxy appears relatively isolated, with the fainter bluer galaxy near it. 
