The galaxy presents as a centrally concentrated, smooth system. The light profile appears relatively uniform, with a high degree of central symmetry. The core exhibits a yellowish-white hue, suggesting an older stellar population. There are hints of a fainter, more diffuse outer region, possibly indicative of an extended stellar halo. The overall structure lacks any obvious spiral arm features or prominent dust lanes, supporting a classification towards the elliptical or lenticular end of the Hubble sequence. Given the smooth light distribution and lack of distinct features, the galaxy appears relatively undisturbed, with no obvious signs of recent merger activity or tidal interactions. There's a very faint, subtle blue-ish tinge at the outermost edges, possibly indicating the presence of a small amount of younger stars, although the overall star formation rate appears subdued.
