The galaxy presents as a relatively smooth, disk-like structure, elongated in shape. There is a noticeable central bulge exhibiting a bright, yellowish-white hue, indicative of an older stellar population. The outer disk displays a gradual color gradient, transitioning from the central yellow to a redder tint towards the edges. This may imply ongoing, but relatively low, star formation activity within the disk. No strong spiral arm structures are immediately apparent, suggesting a potentially late-type spiral or lenticular galaxy. There are no obvious signs of major mergers or significant tidal disturbances. Overall, the galaxy appears to be a relatively massive, well-established system.
