The observed galaxy presents as an elliptical morphology, elongated along its major axis. It exhibits a smooth, centrally concentrated light distribution, indicative of an evolved stellar population. The color gradient is subtle, with a slightly bluer hue towards the outer regions and a redder core, suggesting a possible difference in the age or metallicity of the stellar populations. There is no apparent dust lane or spiral arm structure visible in this image. No significant tidal features or signs of recent merger activity are immediately evident, though subtle disturbances cannot be ruled out at this resolution. The galaxy appears relatively isolated within the field of view.
