The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth, spheroidal morphology with a high degree of central concentration. There is little evidence of spiral arm structure or distinct dust lanes. The object appears elongated, showing a degree of oblateness. The galaxy's core is bright and yellowish-white, suggesting an older stellar population dominating the central region. Moving outward from the core, the color shifts slightly towards green, potentially indicating some ongoing, though subdued, star formation activity in the outer regions. There is no obvious evidence of major mergers or tidal disturbances, though subtle irregularities in the outer envelope cannot be entirely ruled out without further analysis.
