The galaxy presents as an elliptical-like structure, exhibiting a smooth, concentrated morphology. The central region shows a pronounced brightness, suggesting a high density of stars. The galaxy's color profile trends towards the red end of the spectrum. There is little indication of spiral arms or prominent dust lanes, the overall light distribution appears relatively uniform and undisturbed. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape. There is no obvious evidence of ongoing major merger activity. Based on the observed characteristics, the galaxy appears to be a relatively massive system, likely an elliptical galaxy with a population of older stars, and exhibiting low star formation activity.
