The galaxy presents an elliptical morphology, appearing mostly smooth and somewhat elongated. The core exhibits a bright, concentrated luminosity, suggesting a high stellar density. The galaxy displays a yellowish-red hue, which could be indicative of an older stellar population with less active star formation. There are no distinct spiral arms or prominent dust lanes visible, in line with its elliptical classification. There appears to be a second, less concentrated, galaxy in close proximity. There are no signs of significant tidal distortions or major disturbances, it is more likely a minor disturbance. Overall, the galaxy appears to be a relatively evolved system with moderate mass, and subdued ongoing star formation.
