The galaxy presents a generally smooth morphology, with a dominant central bulge characterized by a yellowish hue, indicating an older stellar population. There is little evidence of distinct spiral arm structure or significant dust lanes within the galaxy. The elliptical shape suggests a classification leaning toward elliptical or lenticular, appearing to be in the transition between spiral and elliptical galaxies. There appears to be some degree of low level star formation occurring within the galaxy which is apparent through the reddish edges, but it is unlikely to be a very active star forming galaxy. Overall, the galaxy exhibits a relatively quiescent state with a centrally concentrated light profile. Evidence suggests that there is no major merging event happening to the galaxy at this time. 
