The galaxy presents as a roughly elliptical morphology, exhibiting a smooth, featureless light distribution across its observable structure. The core region shows a concentration of light, gradually decreasing in intensity toward the outer edges. The color appears to be dominated by longer wavelengths, giving it a reddish-yellow hue, possibly indicating an older stellar population. There's no apparent dust lane or spiral arm structure, supporting the classification of a spheroid-dominated system. A subtle asymmetry might be present in the outer regions, but it's within the margin of observational uncertainty. The overall appearance suggests a mature galaxy with limited on-going star formation activity.
