The galaxy presents as a relatively smooth, elongated structure, classified visually as likely elliptical. It exhibits a centrally concentrated luminosity profile, with the core appearing significantly brighter than the outer regions. The major axis is noticeably longer than the minor axis. The galaxy exhibits no prominent spiral arms or significant dust lanes. Faint color gradients appear to be present. The light from this galaxy is redshifted, indicating that it is moving away from us, and is fairly distant. Given the smooth morphology, it is likely that the star formation rate within this galaxy is low. No signs of a major merger are immediately apparent, and there may be minor disturbances, but the galaxy appears largely undisturbed.
