The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated, centrally bright core that gradually diffuses outward into a more indistinct halo. The color profile is relatively uniform, showing a dominant yellowish hue suggestive of an older stellar population. There is no obvious dust lane or spiral arm structure apparent, indicating a lack of significant ongoing star formation. The galaxy appears well-defined and isolated, with no apparent tidal features or signs of recent merger activity. Overall, it seems to be a quiescent and evolved system.
