The galaxy appears to be an elliptical type, exhibiting a generally smooth morphology without distinct spiral arms or a prominent disk. The central region shows a concentrated bright yellowish core, indicating a higher density of older stellar populations. The galaxy's shape is moderately elongated, not perfectly spherical, with an overall yellowish-red hue, suggesting a lack of significant ongoing star formation and a dominance of older, redder stars. There are no obvious signs of major mergers or significant tidal disturbances. The galaxy exhibits a smooth light profile, fading gradually from the center outwards.
