The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a prominent central bulge, characterized by a yellowish-orange hue indicative of an older stellar population. The outer regions appear bluer, suggesting the presence of younger, hotter stars, though the overall color profile leans towards redder wavelengths. The galaxy appears elongated, with a cigar-like shape. There is little evidence of significant dust lanes or prominent spiral arm structures; the galaxy appears largely featureless in terms of distinct morphological details. There is no obvious ongoing merger activity or major disturbance.