The galaxy presents a somewhat irregular, though generally elliptical morphology. Its light distribution is brightest and most concentrated toward the center, decreasing gradually outwards. The overall color appears bluish, suggesting the presence of a younger stellar population and ongoing star formation, although not at a high rate. There is an absence of defined spiral arms or a prominent disk structure. The galaxy's shape suggests it is likely in the process of transitioning from a spiral to elliptical morphology, or is a dwarf elliptical galaxy. There are no clear signs of a major merger event, but a slight asymmetry hints at a possible minor interaction.
