The galaxy presents as a relatively smooth, lenticular or elliptical system, exhibiting a high degree of central concentration. It possesses an overall elliptical morphology, though it appears to be only somewhat rounded rather than perfectly spherical. The light profile suggests a dominant bulge component, with a gradual decrease in luminosity outward from the core. There's a notable lack of distinct spiral arm features or prominent dust lanes, indicating a relatively low level of ongoing star formation. The light emitted is more concentrated in the redder wavelengths. There is a very subtle suggestion of a disk component, but without strong evidence of a spiral structure. No ongoing major merging is present, and any disturbance of the light profile is minimal.
