The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of symmetry. It exhibits a concentrated central bulge that emits strongly across the observed wavelengths. The overall color is distinctly red, with a hint of yellow, suggestive of an older stellar population. The isophotes are generally elliptical and evenly spaced, indicating a lack of significant ongoing mergers or tidal disturbances. The galaxy's apparent elongation suggests an oblate spheroidal shape, viewed at an angle to its rotational axis. There is a subtle decrease in color gradient moving from the core towards the outer edges. No distinct spiral arm structure or dust lanes are visible in this imagery, suggesting a classification towards the earlier end of the Hubble sequence. The galaxy is quite massive with low star formation.