The galaxy presents as a relatively compact object, with a somewhat amorphous appearance. Its color profile suggests a population of intermediate to older stars, exhibiting a general yellow hue. There appears to be some clumpy structure within the galaxy, indicative of either some residual star formation regions, or possibly the after effects of a minor gravitational disturbance from another object. The central region seems marginally brighter, suggesting a concentration of stellar mass or potentially an active galactic nucleus, though the image resolution limits a definitive assessment. Overall, the galaxy appears to be in a transitional phase, exhibiting characteristics between a pure elliptical and a fully developed spiral galaxy.
