The galaxy presents an elliptical morphology, appearing generally smooth and concentrated towards its center. Its color profile is dominated by yellow-red hues, suggesting an older stellar population. There is a subtle gradient from a brighter, more intense central region to a fading, less defined outer halo. Hints of bluer light appear on the edges of this galaxy, possibly due to ongoing star formation, but the bulk of the galaxy is old, suggesting a low star formation rate in its more recent history. There is a small distortion on the edge of the disk, possibly indicating a past or ongoing minor merger. The galaxy does not display a significant amount of dust obscuration.
