The galaxy presents an elliptical morphology, exhibiting a relatively smooth overall appearance with a higher concentration of light towards the center, indicating a prominent galactic bulge. Its shape is elongated, with a cigar-like axial ratio. The color profile suggests a dominant population of older stars, contributing to the yellowish-orange hue observed in the central region, while the outer regions show bluer colors. The galaxy exhibits weak spiral arm features suggesting a spiral galaxy undergoing morphological transformation. No signs of significant tidal disturbances or ongoing major merger events are observed, suggesting the galaxy is relatively undisturbed. The overall morphology indicates the possibility of a lenticular galaxy undergoing passive evolution.
