The galaxy presents as a smooth, elliptical structure with a bright central bulge that dominates the overall light emission. The luminosity decreases gradually from the core outwards, with the isophotes appearing mostly regular and concentric. The galaxy exhibits a slight elongation, with the ratio of the semi-minor to semi-major axis approximately 0.7 to 0.8. There is no distinct spiral arm structure visible, nor is there evidence of significant dust lanes or patches within the galaxy's disk. The color profile appears relatively uniform, with a tendency toward redder hues, especially towards the center of the galaxy, suggesting an older stellar population. There are no discernible signs of ongoing major merger activity or tidal disturbances in the immediate vicinity of the galaxy. The galaxy's effective radius, encompassing half of the total light, is estimated to be around 6 kpc. Overall, this galaxy appears to be a relatively undisturbed elliptical galaxy at a redshift of approximately 0.13.
