This galaxy exhibits a primarily smooth morphology with hints of a possible disk structure. The central region displays a concentrated, bright yellowish-orange hue, suggesting an older stellar population or significant dust obscuration. The galaxy appears elongated, not perfectly spherical, trending towards a cigar shape. There's faint blue light extending from the main body, suggesting some ongoing star formation, albeit at a low rate. There is no strong evidence of major merging activity. The galaxy's moderate size indicates that it is likely a massive galaxy. Overall, it is likely an intermediate spiral, possibly trending towards S0 type, with a substantial spheroidal component.
