The observed galaxy presents as a singular, fairly symmetrical object. The morphology suggests a smooth light distribution, with a concentrated central bulge that dominates the overall luminosity. The galaxy appears roughly elliptical or spheroidal in shape. There is minimal evidence of distinct spiral arms or a well-defined disk structure. The color gradient indicates a population of older stars, particularly concentrated towards the galactic center, as evidenced by the yellowish-white hue. Fainter, bluer regions surrounding the central bulge suggest the presence of a younger stellar population, though these regions are poorly resolved. No significant tidal tails or other signs of recent major merger events are apparent, though there is subtle evidence of a very minor asymmetry on the edges, suggesting the possibility of a past gravitational interaction.
