The galaxy presents as a generally smooth and rounded object with a concentrated central region. The light distribution is relatively uniform, showing no prominent spiral arms or distinct morphological features. The galaxy appears to be a single, coherent object with a possible minor disturbance in the form of a slight extension, suggestive of a weak tidal interaction or recent merger event. The color profile indicates a population of older stars, as evidenced by the reddish-orange hue. Star formation rates appear to be relatively low. Overall, the galaxy likely represents a passively evolving system with significant stellar mass.
