The galaxy presents as a somewhat elongated structure, potentially cigar-shaped, with a slight asymmetry visible in its morphology. The light distribution appears relatively smooth, suggesting a potential lack of prominent spiral arms or distinct features. There is a slight hint of a disturbance in the overall shape, indicative of a possible interaction with another galaxy or a minor internal disruption. The galaxy's color profile is dominated by redder hues, indicative of an older stellar population and comparatively low levels of recent star formation. The core region appears brighter and more concentrated, possibly indicative of a significant bulge component. The estimated size suggests that we're observing a galaxy of considerable extent. While not definitively a merger, there is a subtle irregularity that warrants further investigation into potential tidal interactions or previous merger events.
