The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light profile suggests an elliptical shape, appearing nearly circular in projection. The core exhibits a bright, yellowish hue, possibly indicative of an older stellar population. Moving outward from the core, the color transitions to a slightly redder shade, suggesting a mixture of stellar ages, but generally consistent with aging stars and low star formation rates. No distinct spiral arm structure or prominent dust lanes are visible within this image, which is consistent with it being a galaxy lacking significant ongoing mergers or disk presence. Small disturbances may be occurring, however the galaxy is mostly relaxed.
