The galaxy presents a generally smooth and rounded morphology. Its light profile suggests a centrally concentrated structure with a gradual decline in luminosity outward. The core region exhibits a bright, diffuse glow, transitioning to a slightly fainter outer halo. There is no obvious presence of spiral arms, bars, or prominent dust lanes. Based on the color distribution, the galaxy appears to be dominated by older stellar populations, exhibiting a yellowish hue throughout the majority of its visible structure. There is little to no evidence of ongoing major star formation, consistent with a relatively quiescent state. Minor disturbances or interactions with other galaxies seem to be absent. The galaxy appears to be a relatively isolated system, exhibiting a classical elliptical or lenticular morphology.
