The galaxy presents as a relatively compact object. It appears largely smooth in overall morphology, with a high degree of central concentration. There is little discernible structure in the form of spiral arms or a prominent disk. The color profile suggests a dominant population of older stars, contributing to its relatively red appearance. A slight elongation is detectable, with an approximate elliptical shape, suggesting it may be a late-type spiral galaxy. The galaxy exhibits some characteristics of star formation, as indicated by a faint blueish hue present in the galactic center. There are no obvious signs of recent major mergers or tidal disturbances, with only slight irregularities.
