The galaxy appears to be a relatively smooth, disk-like structure, likely a spiral galaxy viewed at an angle. The central bulge is bright and concentrated, exhibiting a yellowish hue, possibly indicative of an older stellar population. Moving outward from the bulge, a bluer disk is present, suggesting the presence of younger stars and ongoing star formation. There is a slight hint of disturbance or asymmetry in the outer regions of the disk, with one side appearing more extended or diffuse than the other. There is no prominent tidal tails or other major distortions, although the asymmetry could point to a minor interaction or recent accretion event. Overall, the galaxy displays characteristics of both elliptical and spiral galaxies, presenting a transition between the two morphologies. 
