The galaxy presents as an elliptical morphology, exhibiting a smooth and centrally concentrated luminosity profile. Its shape is somewhat elongated, with a cigar-like appearance. The color gradient suggests a population of older stars, with a yellowish central region gradually fading to a redder hue at the outer edges. There appears to be little or no evidence of ongoing star formation. No significant signs of tidal disturbances or mergers are detected. The galaxy exhibits no spiral arm structures or prominent dust lanes.
