The galaxy appears to be an elliptical or lenticular type, exhibiting a predominantly smooth morphology. It displays a moderately elongated shape, leaning towards a cigar-like appearance. The color profile suggests an older stellar population, with a subtle reddish hue. There is very little evidence of spiral arm structure, and a notable lack of dust lanes, consistent with a more evolved system. There may be a very small amount of minor disturbance, but it appears to be mostly self contained. The central bulge is prominent and appears to dominate the overall light output of the galaxy. There are not many areas where active star formation is suspected to be ongoing. 
