The galaxy presents a generally smooth morphology, appearing elliptical in shape. The light is concentrated in the center of the galaxy, with a gradual decrease in luminosity towards the outer regions. The color profile suggests a predominantly older stellar population, with a yellow-red hue indicative of evolved stars. There is little evidence of strong spiral arm structures or prominent dust lanes. Based on the generally smooth appearance, the object is more consistent with an elliptical galaxy than a spiral galaxy. There appears to be no significant disturbance indicative of an ongoing major merger. Any evidence of tidal tails or other interactions is not immediately apparent in the image. The concentration of light and overall smooth structure supports the classification of this galaxy as an elliptical or lenticular type.
