The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a high degree of central concentration, with light intensity decreasing gradually from the core outwards. There appears to be a lack of significant spiral arm structures or prominent dust lanes. The galaxy's color appears to be yellowish, suggesting an older stellar population dominated by redder stars. No obvious signs of ongoing major merger activity or tidal disturbances are apparent, although a subtle asymmetry cannot be entirely ruled out. The overall impression is that of a mature galaxy with a substantial stellar mass and a relatively low star formation rate.
