The galaxy presents as a lenticular or possibly elliptical form, with a generally elongated, cigar-shaped appearance. Its light distribution appears relatively smooth and concentrated, with no distinct spiral arm structures visible. A slight color gradient can be observed, with a central region showing a more yellowish or reddish hue, potentially indicating an older stellar population. The outer regions display a bluer color. This suggests the presence of younger stars and ongoing star formation. There is a possibility of a minor interaction or disturbance affecting the galaxy's shape. The overall morphological assessment points toward a galaxy that is in a relatively late stage of its evolution, with potentially diminishing star formation activity but some ongoing star formation. Its overall size is moderate.
