The galaxy presents as an elongated, cigar-shaped structure. It exhibits a smooth, featureless morphology with a central concentration of light that gradually diffuses outwards. The color profile indicates a dominance of light at shorter wavelengths, with a blue-white hue. This suggests a population of younger, hotter stars. There is no evidence of distinct spiral arms or a prominent central bulge. Faint hints of possible minor tidal disturbances are observed, potentially suggestive of an interaction, although this feature could be simply a result of the elongated shape of the galaxy. There does not appear to be any dust absorption or obscuration within the system. Overall, the galaxy appears as an elliptical or lenticular galaxy undergoing active star formation.
