The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a high degree of luminosity, decreasing radially outward. The overall shape appears somewhat elongated, deviating from a perfectly circular profile. There is no obvious spiral arm structure or prominent dust lanes visible in this image. Faint extensions hint at a possible halo, though definitive determination is limited by image resolution. The color appears generally consistent across the galaxy, showing a redder spectral profile without clear evidence of distinct blue star-forming regions. The galaxy is isolated, showing no evidence of a major merger event in the image.
