The galaxy presents as a singular, relatively smooth object with a concentrated central bulge and a diffuse halo. The overall shape approximates a spheroid, exhibiting minimal deviation from a circular form. The galaxy's color profile is predominantly yellow, suggesting an older stellar population. The absence of distinct spiral arms or dust lanes indicates a lack of significant ongoing star formation within the galaxy. There is no apparent evidence of tidal tails or other morphological distortions that might suggest recent merger activity, although there may be a minor disturbance. The galaxy exhibits a luminosity consistent with other galaxies within its redshift range. Its observed characteristics suggest a relatively high mass concentration.
