The galaxy presents as a moderately compact object with a concentrated central bulge. The light profile appears relatively smooth, with a gradual decrease in intensity from the core outward. The shape is generally rounded, exhibiting a slight elongation, but without prominent features indicative of a strong bar or spiral arm structure. There is a hint of disturbance in the surrounding halo, with a subtle, irregular distribution of light, suggesting a potential minor interaction or past merger event. Color gradients are present, with the central region exhibiting a yellowish hue, possibly indicating an older stellar population, while the outer regions appear slightly bluer, suggesting the presence of younger stars. Overall, the galaxy appears to be relatively isolated with a smooth morphology. 
