The galaxy presents a generally smooth morphology, with a high degree of central concentration of light. The color profile shows a prominent yellow hue, suggesting an older stellar population with a paucity of ongoing star formation. There is very weak evidence for any defined spiral structure or prominent disk-like morphology, it appears mostly spheroidal. It presents a slightly elliptical appearance, deviating moderately from a perfectly circular form. There's no strong evidence of major tidal disturbances or ongoing merger activity, though some faint irregular features could indicate past minor interactions or internal instabilities.
