The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth and concentrated light distribution. It has a notable central bulge, characterized by a bright yellowish-orange hue. The overall shape is largely round, showing minimal signs of significant tidal disturbances or ongoing merger activity. There is a faint outer halo or envelope surrounding the central region, though the light is diffused and decreases in intensity with radial distance. Based on the observed color, the stellar population is likely dominated by older stars, indicating a relatively low rate of current star formation activity.
