The galaxy presents as a relatively smooth, elliptical structure. It appears to be an early-type galaxy, likely an elliptical or lenticular galaxy, with a concentrated central bulge that exhibits a yellowish hue. This suggests an older stellar population within the core. The outer regions of the galaxy gradually fade into the background, exhibiting a slightly bluer tint, perhaps indicating a small amount of younger stars or ongoing star formation. There is no evidence of strong spiral arm structures or prominent dust lanes. The overall morphology is consistent with a non-disturbed system, showing no obvious signs of recent or ongoing major mergers. The galaxy is elongated, exhibiting an intermediate axis ratio. 
