The galaxy presents as a luminous, elongated structure. The central region exhibits a high degree of smoothness with an orange/yellow hue, suggestive of an older stellar population. The overall shape approximates a flattened spheroid. The outer regions show a subtle greenish tint, possibly indicating areas of more recent star formation, although the smoothness suggests that it is not strong. There is no clear indication of spiral arms or a bar. It appears relatively isolated, with no obvious signs of recent or ongoing major mergers, though some minor disturbances or tidal features cannot be ruled out, given the somewhat irregular boundary. The galaxy's overall morphology suggests an elliptical classification, or potentially a lenticular galaxy viewed at an angle.
