The galaxy presents a smooth, elliptical morphology. The light distribution appears centrally concentrated with a gradual decrease in intensity moving outwards, showing no distinct spiral arm structure or prominent disk. It has an overall yellow/orange hue, suggesting an older stellar population with a relatively low rate of ongoing star formation. The galaxy appears somewhat elongated, displaying an axis ratio indicating a non-spherical shape. There is no obvious evidence of recent merger activity or significant tidal disturbances, and the galaxy does not appear to be undergoing any major interactions.
