The galaxy appears to be a relatively small, elongated elliptical galaxy at a redshift of approximately 0.05. It presents a smooth, featureless morphology with a central concentration of light that fades gradually towards its edges. The galaxy exhibits a bluer hue in its central regions, suggesting the presence of a population of younger, hotter stars, although the overall star formation rate is likely low. There is no discernible evidence of spiral arms, a prominent disk, or ongoing major mergers. The galaxy's shape is cigar-like, indicating a significant ellipticity. Small tidal disturbances can not be ruled out but are unlikely.
