The galaxy presents a generally smooth morphology, with a slightly elongated, cigar-shaped appearance. The light distribution appears centrally concentrated, fading gradually towards the edges. There is very little evidence of spiral arm structure or significant dust lanes. The color is predominantly yellowish, suggesting an older stellar population, with a potential paucity of recent star formation. The overall structure indicates a relatively evolved system, exhibiting some characteristics of an elliptical or lenticular galaxy. There appears to be no major ongoing merger activity, although there might be very minor asymmetry that may be suggestive of a minor disturbance.
