The galaxy presents a relatively smooth, elliptical morphology. The light distribution appears centrally concentrated, with a gradual falloff in intensity towards the outer regions. There is little evidence of spiral arm structures or significant dust lanes. The galaxy exhibits a yellowish-orange hue, suggesting an older stellar population with a lower rate of on-going star formation. The galaxy appears to be relatively isolated, with no obvious signs of a recent or ongoing major merger. However, there is a suggestion of some minor tidal disturbance in the form of faint extensions, potentially indicating a past interaction.
