This galaxy presents as an elliptical-like system, characterized by a notable lack of distinct spiral arm structures. The light distribution is centrally concentrated, with a smooth radial falloff. The core region exhibits a yellowish hue, suggesting an older stellar population dominated by evolved stars. Moving outward from the core, the color gradually shifts to a slightly bluer shade, which may indicate the presence of younger stars or ongoing, albeit minimal, star formation activity. The overall shape appears elongated, deviating slightly from a perfect sphere, but is more consistent with an elliptical or lenticular morphology. There is no strong evidence of significant tidal disturbances or ongoing major merger events. The galaxy exhibits a fairly quiescent state, indicative of a system where star formation has either ceased or is occurring at a very low rate.
