This galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated morphology. The light profile suggests a relatively featureless structure, lacking prominent spiral arms or distinct dust lanes. The galaxy's shape is elongated, displaying a cigar-like appearance rather than a perfectly circular form. A slight asymmetry is perceptible in the outer regions. The color gradient indicates a redder core, potentially indicative of an older stellar population, gradually transitioning to slightly bluer hues in the outskirts, which may suggest ongoing, albeit low, levels of star formation in the outer regions. There is no apparent evidence of significant tidal disturbances or merging activity, although a subtle irregularity in the halo cannot be ruled out. The overall impression is that of a mature galaxy undergoing slow, quiescent evolution.
