The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated luminosity profile. The light is dominated by redder wavelengths. There may be a slight hint of a disk. There are no strong indications of recent or ongoing major merger activity. The system shows a moderate projected size, with no resolved spiral arms or prominent dust lanes visible at this resolution. The galaxy exhibits a degree of roundness, deviating from a perfectly spherical shape. Some minor disturbance is present, with some asymmetrical light distribution. Based on its redshift, this is a relatively distant object. The stellar population is likely composed predominantly of older, redder stars, with a low rate of current star formation.
