The galaxy appears to be an elliptical type, with a smooth, largely featureless structure. The light profile displays a concentrated central bulge which indicates a high stellar density towards the core, with a gradual decrease in luminosity towards the outer regions. The shape is moderately elongated, presenting an intermediate axis ratio that might imply a classification between E3 and E5 on the Hubble sequence. The color gradient suggests that the central bulge might be populated by older, redder stars, whilst the outer regions exhibit a slightly bluer hue, hinting at a younger stellar population or the presence of some star formation, though not prominently. There is no clear evidence of spiral arms or a disk structure, but there are some indications of minor disturbance in the morphology, suggesting a possible past interaction or minor merger event. 
