The galaxy presents a generally smooth morphology, appearing largely featureless in this image. It exhibits a spheroidal shape, tending towards round rather than elongated. The light distribution is concentrated in the center, suggesting a prominent galactic nucleus. The color profile indicates a population of relatively old stars, contributing to its reddish hue, particularly when compared to bluer, younger star-forming regions. Despite its overall smooth appearance, there is faint evidence of some minor structural irregularity. The absence of strong spiral arms or a distinct disk further supports its classification as an elliptical or lenticular galaxy at redshift z=0.326. It is not currently undergoing a major merger or significant tidal disturbance.
