The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless profile. The central bulge dominates the galaxy's structure, displaying a concentrated, bright yellowish-white luminosity indicative of an older stellar population. Progressing outwards from the core, the light gradually decreases. The galaxy's apparent shape is elongated, suggesting it is viewed at an angle relative to its equatorial plane. There is a subtle color gradient, with the outermost regions showing a slight hint of bluer tones, potentially indicating the presence of a younger population of stars, albeit in comparatively small quantities. There are no prominent spiral arms, dust lanes, or other distinct features, reinforcing its classification as an elliptical galaxy.
