The galaxy presents as an elliptical morphology with a moderate redshift. Its overall structure appears to be relatively smooth, exhibiting a central bulge with what looks like a faint, extended disk. The bulge exhibits an orange-red hue, indicative of an older stellar population. Fainter regions within the disk have a more blue-green tint, suggesting the presence of some younger stars and possibly some ongoing star formation, although limited. The galaxy appears elongated, almost cigar-shaped, and shows some indications of a possible minor disturbance or interaction, though no major merging is apparent.
