The galaxy presents a largely elliptical morphology with a high degree of central concentration. It exhibits a smooth, featureless profile in this image, with a minimal presence of distinct spiral arms or dust lanes visible at this resolution. The overall color index shows a tendency toward redder hues, suggesting a population of older stars and relatively low ongoing star formation. The light distribution appears fairly uniform without any pronounced irregularities or tidal features that would indicate recent merger activity. The galaxy appears somewhat inclined from our line of sight.
