The galaxy exhibits an elliptical morphology, with a smooth, centrally concentrated light distribution. It appears to be relatively isolated, showing no obvious signs of ongoing major mergers or tidal interactions. The galaxy has a noticeable reddish hue, suggesting a population of older stars and potentially lower star formation activity. The lack of prominent spiral arms or significant dust lanes further supports its classification as an elliptical galaxy at a redshift of approximately 0.123.
