The galaxy presents an elliptical morphology, appearing as a smooth, elongated spheroid. The light distribution appears centrally concentrated with a gradual decline in brightness from the core outwards. There is a slight elongation visible, suggesting a non-spherical shape but it mostly falls under an "in between" roundness. The color profile is somewhat homogenous, with a tendency towards redder hues, hinting at an older stellar population and relatively low ongoing star formation activity. No prominent spiral arms or distinct dust lanes are discernible. The galaxy appears relatively isolated with no signs of major ongoing merger activity or tidal disturbances.
