The galaxy presents as an elliptical morphology with a high degree of central concentration. A bright, compact core dominates the galaxy's overall luminosity profile, exhibiting a yellow-white hue, suggesting an older stellar population within the core. The galaxy's outer regions appear to have a smoother, more diffuse structure, which gradually fades into the background. The overall shape is elongated, with an ellipticity of approximately 0.7. There may be a faint disk component present, but it's not distinctly defined, suggesting that the galaxy is likely dominated by a spheroidal component with little to no prominent spiral arms. The color appears to be more red towards the center, and bluer toward the edges, suggesting more active star formation is located on the edges, or that they are less obscured by dust.
