The observed galaxy exhibits a prominent spiral structure, characterized by two well-defined arms emanating from a central bulge. The arms display a moderate winding, neither tightly coiled nor loosely extended. The bulge appears to be of moderate size, neither dominating the overall structure nor being negligibly small.  There is a suggestion of a bar structure present, though it doesn't appear very strong. The galactic disk is not seen edge-on, and shows no obvious signs of major merger activity, although there may be some signs of disturbance. Color gradients within the galaxy are evident, with the central bulge exhibiting a yellowish hue, likely indicating an older stellar population. The spiral arms display bluer tones suggesting ongoing star formation activity.
