This galaxy appears to be a relatively smooth, elongated system, presenting an edge-on or highly inclined disk. The central bulge is not highly pronounced, exhibiting a diffuse glow transitioning into the fainter outer regions. The light distribution suggests a higher concentration of older stellar populations in the bulge, fading towards the edges, with some evidence of dust lane absorption bisecting the main axis. Overall the shape and composition aligns to a disk-like structure, and it does not show any indication of ongoing major merging activity or significant tidal disturbances. The galaxy exhibits redder hues and is a smaller, more compact structure.