The galaxy presents a primarily smooth morphology, with no discernible spiral arms or bar structure visible in this imaging. Its light distribution appears centrally concentrated, indicating a spheroid-dominated system. The galaxy exhibits a yellowish hue overall, potentially suggestive of an older stellar population and a lower rate of on-going star formation. The round shape of the object is clear in the image. There is no sign of any merging activity or major disturbances in its morphology.
