The galaxy presents as a largely featureless, elliptical morphology. Its light profile is dominated by a smooth, centrally concentrated bulge. A subtle color gradient is observed, with the core exhibiting a more yellowish hue transitioning to a slightly redder outer halo. No prominent spiral arms or distinct dust lanes are discernible. There is very little, if any, evidence of active star formation across the galaxy. The overall appearance suggests a relatively evolved stellar population and a quiescent state. A slight asymmetry in the color distribution on the lower right quadrant hints at a possible minor interaction or tidal disturbance in its past, although this is difficult to assert with certainty. The galaxy appears to be relatively isolated, lacking close companion galaxies that would suggest recent or ongoing major merger activity.
