The galaxy presents as a relatively smooth, elliptical morphology with a concentrated central bulge. The light distribution appears centrally dominated, decreasing steadily outwards without prominent spiral arm features or significant dust lane obscuration. The galaxy exhibits a yellowish hue in its core, suggesting an older stellar population, with slightly bluer tones towards the outer regions. The observed color gradient implies ongoing, albeit perhaps subdued, star formation activity. No apparent tidal features or signs of major mergers are visible in this single image. The isophotes appear generally regular, with a high degree of roundness.
