The galaxy presents as a relatively smooth, elliptical or lenticular morphology, exhibiting a concentrated central bulge. The color profile suggests an older stellar population, dominated by redder wavelengths. There are no clear spiral arm structures or significant dust lanes visible. The overall shape is approximately rounded, with a slight deviation towards a more elongated form. There's no significant visual evidence of ongoing major merger activity or tidal disturbances, although minor asymmetries cannot be ruled out at this resolution. The light profile appears to gradually fade outwards from the core, without distinct breaks or sharp edges.
