The galaxy appears as a centrally concentrated object, with a generally elliptical morphology. The light distribution is smoother than that of a typical spiral galaxy, suggestive of a higher fraction of older stellar populations or a more spheroid-dominated system. A very slight extension is visible along the vertical axis of the galaxy. The colors within the galaxy's central region display a strong red-orange hue, potentially indicating a significant population of older stars and/or dust obscuration. Fainter bluer tones appear in the disk region, implying some ongoing star formation in the outer reaches. There is no distinct spiral arm structure visible. Overall, it resembles a massive galaxy at intermediate redshift, possibly undergoing morphological transformation or quiescence. The overall shape indicates it is somewhere between a completely spherical galaxy and a cigar-shaped one. There are some small disturbances potentially indicating some merger activity or tidal forces.
