The galaxy presents as an elliptical type, with a notable smooth, centralized bulge exhibiting a dominant yellow-orange hue, suggesting an older stellar population. A faint, diffuse disk surrounds the bulge, displaying a slight inclination relative to our line of sight. There is a minor hint of blue within the disk. No prominent spiral arm structures are discernible; instead, a subtle, amorphous feature extends from one edge of the disk, possibly indicating a tidal interaction or minor disturbance. Overall, the galaxy appears relatively isolated, with no significant signs of ongoing or recent major mergers, but perhaps minor interaction.
