The galaxy presents a primarily smooth, elliptical morphology. The light profile exhibits a concentrated central bulge that diminishes gradually outward, suggesting an older stellar population dominating the galaxy. A subtle bluer hue is observed in the outer regions of the disk, possibly indicative of recent, low-level star formation or a younger stellar population compared to the central bulge. No spiral arm structures or significant dust lanes are discernible in the image. The overall structure indicates a galaxy in a relatively quiescent state. There is a slight suggestion of minor tidal disturbances and a faint plume extending from the main body, hinting at a possible past merger event or gravitational interaction with a nearby galaxy. The galaxy appears fairly isolated in the image, with no other large galaxies nearby to cause strong tidal effects.
