The galaxy presents as a centrally concentrated object with a relatively smooth and luminous profile. The core region is bright and appears nearly spherical, while the outer regions fade gradually into the background. There is very little indication of spiral arm structure or significant morphological features such as dust lanes or irregular shapes. The overall impression is that of an elliptical galaxy, possibly an early-type spiral with a dominant bulge and tightly wound arms viewed at a distance. The light from the galaxy is dominated by a yellowish-white hue, suggesting an older stellar population with a low rate of recent star formation. There is no apparent evidence of ongoing merger activity or significant tidal disturbances.
