This galaxy presents an overall elliptical morphology, though some asymmetry is apparent, possibly indicating a past or ongoing interaction. The central region exhibits a concentrated luminosity profile, appearing relatively smooth and featureless, characteristic of an older stellar population. Moving outwards from the center, a subtle disk-like structure becomes visible, although it lacks the defined spiral arms typical of disk galaxies. The color gradients suggest a radial variation in stellar population, with the central bulge appearing redder than the outer regions. The outer disk exhibits faint blue hues. This potentially indicates the presence of younger, hotter stars in these areas. There are no clearly defined dust lanes or prominent star-forming regions visible in this image. The galaxy's morphology places it somewhere on the spectrum between an elliptical and a spiral galaxy, but there are subtle signs of it being more than just a simple Elliptical galaxy.
