The galaxy presents a largely smooth and featureless morphology. It exhibits a centrally concentrated luminosity profile, appearing brightest at its core, with the light intensity gradually decreasing towards the outer regions. The overall shape appears predominantly round, with only subtle deviations from perfect circularity. There is no clear evidence of spiral arm structures or a well-defined disk. There are no obvious signs of recent or ongoing major mergers, tidal tails, or other significant disturbances in its structure, though some minor asymmetry cannot be ruled out. The galaxy has a yellow-reddish hue, suggesting an older stellar population. It is relatively large for a galaxy, which is also an indication that it is a galaxy of significant mass. The observed light output, while not excessively faint, suggests a relatively low current star formation rate within the galaxy.
