The galaxy presents as a somewhat elliptical structure. Its core region exhibits a concentrated luminosity, suggesting a significant population of stars and possibly an active galactic nucleus. There are indications of a slight disturbance or potential merger event occurring with what appears to be a smaller companion galaxy or tidal debris in close proximity. The overall color profile of the galaxy leans toward a yellowish-orange hue, which would suggest an older stellar population with a reduced rate of active star formation throughout the main body. However, there also appears to be a small pocket of blue emission, hinting at more recent star formation in that localized area.
