The galaxy presents a generally smooth morphology, suggestive of an elliptical or lenticular classification. The light distribution appears centrally concentrated, exhibiting a prominent, bright core indicative of a bulge component. There is a subtle, diffuse halo surrounding the core, fading gradually into the background. The color profile suggests a relatively uniform stellar population, with a slightly bluer hue in the outer regions. While predominantly smooth, a subtle irregularity or distortion in the galaxy's outer envelope is visible, possibly signifying minor tidal disturbances or past merger events. There are no apparent spiral arm structures or prominent dust lanes discernible at this resolution.
