The galaxy appears to be an elliptical type, exhibiting a generally smooth light distribution across its structure. The core presents a bright, concentrated luminosity with a yellowish hue, indicative of an older stellar population. Extending outwards from the core, the galaxy's halo demonstrates a gradual decrease in luminosity. A subtle color gradient is observed, with the outskirts appearing slightly redder compared to the central region. The overall shape is elongated, but not strongly so, appearing closer to round. There may be minor disturbances or faint tidal features suggesting a possible interaction or past merger event. The galaxy shows evidence of a limited rate of star formation.