The galaxy presents as a flattened spheroid, appearing somewhat cigar-shaped in its overall form. Its color profile indicates a dominance of older stellar populations, with the central bulge exhibiting a more pronounced yellowish hue. The outer regions appear slightly bluer, suggesting the presence of younger stars. The galaxy’s surface brightness appears relatively smooth, hinting at a lack of significant spiral arm structure. There are only minor indications of disturbances or ongoing mergers, and a general lack of clumpy structures or bright knots, implying a relatively quiescent state of star formation. The galaxy's overall appearance suggests a morphological classification somewhere between an elliptical and a lenticular galaxy.
