The galaxy presents as an elliptical morphology, displaying a smooth and centrally concentrated light distribution. The central region exhibits a bright, yellowish-golden hue, suggesting a population of older stars. The luminosity gradually decreases with radial distance from the core. There is a subtle, extended halo surrounding the central bulge, also displaying a smooth texture without any distinct spiral arms or prominent dust lanes. The overall shape is moderately elliptical, not perfectly spherical, but also not highly elongated. No signs of major tidal disturbances, merging events, or active star formation regions are readily apparent in the image. Based on these characteristics, a classification towards the elliptical end of the Hubble sequence, with no clear evidence of recent interactions, seems appropriate.
