The galaxy presents an elliptical morphology, appearing largely smooth and rounded. It is characterized by a concentrated central bulge that emits a yellow-orange light. There is a subtle color gradient from the core outwards, which suggests the presence of an older stellar population. The overall structure indicates a system dominated by random stellar orbits, with little evidence of spiral arms or significant disk features. There is no clear indication of strong recent merger activity or tidal disruptions affecting the galaxy's overall shape. It appears as an isolated system with minimal visible signs of disturbance.
