The galaxy presents an elliptical morphology, appearing elongated with a distinct central bulge. The core exhibits a yellowish-orange hue, indicative of an older stellar population. Fainter, diffuse emission extends outwards from the core, gradually fading into the background. There appears to be a slight disk-like structure, although the galaxy lacks prominent spiral arms. A subtle blue tint around the outer edges suggests the presence of younger, hotter stars in the galaxy's periphery, indicating ongoing, albeit low, star formation activity. No significant tidal features or signs of major mergers are readily apparent in this image.
