This galaxy presents as an elongated, cigar-shaped structure. It appears predominantly smooth in texture, lacking any distinct spiral arms or bar features. The central region displays a concentrated brightness, suggesting the presence of a substantial galactic bulge or a central supermassive black hole actively accreting matter. The color gradient shifts from a yellowish hue in the center to a slightly bluer tone towards the outer edges, potentially indicative of younger stellar populations or ongoing star formation in the periphery. There are no obvious signs of tidal disturbances or interactions with neighboring galaxies, which suggests it is a relatively isolated system. The galaxy's overall form is consistent with an elliptical morphology, though a classification as a lenticular galaxy cannot be entirely ruled out without further spectroscopic analysis.
