The galaxy presents a predominantly smooth morphology, appearing largely featureless without significant spiral arm structures or a prominent central bar. Its overall shape is elliptical, tending toward a circular appearance, though the possibility of a slight elongation cannot be entirely discounted given the image resolution. The color profile suggests a concentration of older stellar populations, characterized by a yellowish-red hue in the central region, indicative of evolved stars. While the primary body of the galaxy exhibits uniformity, there are hints of minor disturbances or interactions, suggesting a potential past merger event or ongoing gravitational influence from nearby galaxies, albeit with low significance in the current image. No significant dust lanes or active star-forming regions are immediately apparent, leading to the conclusion that the galaxy's star formation rate is relatively quiescent. Overall, it presents as a mature and well-formed galaxy in a late stage of its evolutionary timeline.
