The galaxy presents as a relatively smooth, centrally concentrated object. The morphology appears to be largely spheroidal, with a high degree of central symmetry. The color profile exhibits a yellow-red hue, suggesting an older stellar population. There are faint extensions, potentially tidal features, in the halo. The image lacks high-resolution detail, precluding definitive classification, but it appears to be a fairly massive galaxy with a low star formation rate. No strong evidence of spiral arms or a pronounced disk structure is apparent. There is no obvious indication of a major ongoing merger, though subtle irregularities could indicate past interactions.
