The galaxy presents as a relatively smooth, concentrated object. It exhibits a generally elliptical morphology, appearing nearly circular in projection. The color profile suggests an older stellar population, with a dominant yellowish hue. There is little evidence of significant dust lanes or prominent spiral arm structures. Faint, diffuse outer regions are visible surrounding a brighter, more compact core. There does not appear to be any significant ongoing merging activity or major disturbances to the overall structure. The galaxy is likely an early-type galaxy, possibly an elliptical or lenticular, with a moderate stellar mass and relatively low star formation rate.