The galaxy presents as a relatively elongated, disk-shaped structure. The primary axis of the galaxy appears to be significantly longer than its minor axis. The central region exhibits a pronounced concentration of light, likely indicative of a galactic bulge. The galaxy displays a color gradient, transitioning from a bluer hue in the inner regions to a redder hue at the outskirts. Faint arms are present, but not well-defined. There are some irregular features, particularly on the outer regions of the disk, indicating the possible presence of minor tidal disturbances or ongoing interactions. The overall appearance suggests an older stellar population with low ongoing star formation.
