The galaxy presents as an elongated, cigar-shaped structure. Its light distribution is relatively smooth, with a centrally concentrated luminosity that decreases gradually towards the outer edges. There is a slight color gradient visible, with the central region appearing more yellow/red, potentially indicating an older stellar population. The outer regions have a hint of blue. No distinct spiral arm structures or prominent dust lanes are discernible within the galaxy's morphology. The overall appearance is consistent with an elliptical or lenticular galaxy, with no strong signs of active star formation. There appears to be a possible interaction or merging event with a second galaxy that has a similar morphology.
