The galaxy presents as a relatively bright, centrally concentrated object. Its morphology appears smooth and largely featureless, displaying a high degree of radial symmetry. The overall shape approximates a circular form, with minimal elongation detected. There is no obvious spiral arm structure visible in the image, nor is there evidence of a prominent disk. The galaxy's color suggests an evolved stellar population, potentially dominated by older, redder stars. There is a hint of a fainter structure slightly offset from the center of the galaxy; this could suggest a minor tidal disturbance, a satellite galaxy, or some other irregularity. No prominent dust lanes or regions of intense star formation are discernible. The appearance is consistent with an elliptical galaxy that might be undergoing or have undergone a minor interaction.
