The galaxy presents an overall reddish hue, which could indicate an older stellar population. The galaxy appears relatively smooth in morphology, suggesting a possible elliptical or lenticular classification, although some disk features cannot be ruled out given the resolution. There are potential signs of minor disturbances, indicating the possibility of past or ongoing interactions with other galaxies. There appears to be ongoing star formation, albeit potentially at a lower rate. The galaxy's structure is moderately elongated.
