The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a high degree of central concentration. The color profile suggests a population dominated by older stars, trending towards redder hues in the central region. There is a lack of prominent spiral arm structure or significant dust lanes. The galaxy exhibits a moderate ellipticity, appearing slightly elongated rather than perfectly spherical. There is no visually apparent sign of ongoing major merging activity or significant tidal distortions.
