The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears yellowish-white in color, suggesting an older stellar population. The galaxy's overall shape is elongated, leaning towards a cigar-like appearance, and it is oriented at an angle relative to our line of sight. There is a subtle transition from the bright central bulge to a fainter, less defined outer halo. No distinct spiral arms or significant dust lanes are discernible. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances, although a minor disturbance cannot be ruled out. There is minimal evidence of active star formation within the observable spectrum.
