The galaxy presents as a well-defined, elongated structure. It is strongly cigar shaped. There is not a strong central bulge, rather a smooth, diffuse light distribution. The galaxy exhibits a lack of spiral arm structure, appearing largely featureless in terms of organized star formation regions. The color profile suggests a lack of recent star formation, trending towards redder hues across the body of the galaxy. It appears to be a relatively isolated object with no major interacting galaxies nearby. There may be some minor disturbances to the galaxy's disk, but these are minimal. Overall, the galaxy appears to be a relatively quiescent system, likely an elliptical or lenticular type, with an estimated mass of around 10^10.5 solar masses.
