The galaxy presents as a lenticular or early-type spiral system, characterized by a dominant bulge and a faint, elongated disk. The overall color index suggests a population of older stars, with a redder appearance indicative of lower recent star formation activity. The disk appears relatively smooth with no prominent spiral arm structure visually discernible in this image, which implies a lack of significant gas and dust content. The galaxy's elliptical shape and the lack of obvious disturbances suggest a relatively relaxed morphology, with no signs of recent major merger events. There is a slight asymmetry to the disk suggesting possible minor interaction.