The observed galaxy presents a generally smooth, elliptical morphology. There is a concentrated central bulge region exhibiting a yellowish hue, suggesting an older stellar population dominating the core. Surrounding the core is a diffuse halo exhibiting a bluer color. The ellipticity of the galaxy appears moderate. Faint, ill-defined features may suggest minor disturbances. Overall, the galaxy's light distribution is relatively even. There does not appear to be significant presence of dust lanes or prominent spiral arm structures.
