The galaxy presents as a smooth, elliptical morphology, elongated in shape with a high degree of axial ratio. The central region exhibits a higher surface brightness concentration, indicative of a bulge component. There is a lack of apparent spiral arm structure or prominent dust lanes. The overall color appears to be a relatively uniform bluish-white, suggesting a stellar population that is not dominated by older, redder stars, however, there is not a lot of distinct color information present. There are no signs of significant tidal disturbances or ongoing major merger events. Based on these characteristics, this galaxy appears to be a relatively isolated, early-type spiral galaxy.
