The observed galaxy presents a structure with a relatively smooth central bulge, exhibiting a bright, concentrated core region. Emerging from this central area is a discernible, yet somewhat ill-defined, disk component. This disk appears to be oriented edge-on relative to the observer's line of sight.

The color profile shows a gradient, with the central bulge exhibiting a bluer hue indicative of younger stellar populations, while the disk displays a slightly redder color, potentially suggesting older stars or dust obscuration. There may be some minor disturbances in the disk structure. The outer regions of the galaxy appear faint, gradually fading into the background sky. Overall, this galaxy appears to be undergoing a period of relative quiescence, with no strong indications of major mergers or significant star formation activity.
