The galaxy appears to be elliptical in shape, with a smooth, concentrated light profile suggesting an early-type classification. The core exhibits a bright, yellowish hue, likely indicative of an older stellar population. Moving outward, the galaxy's luminosity gradually diminishes. There may be some very faint disturbances or tidal features, but the overall morphology suggests it's a relatively relaxed system, not currently undergoing a major merger event. The colors suggest a lack of significant ongoing star formation.
