The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated distribution of light. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. The galaxy exhibits an overall elliptical shape, with the light intensity gradually decreasing from the center towards the outer regions. There are no visible spiral arms, dust lanes, or other distinct features typically associated with spiral galaxies. There are no clear signs of on-going or recent major merger activity. A slight asymmetry in the outer regions might indicate a minor interaction.
