The galaxy presents a generally smooth and rounded morphology, suggesting a likely elliptical classification, or possibly a spiral viewed face-on with poorly defined spiral arms. The light distribution is concentrated towards the galactic center, exhibiting a bright, prominent core. The color appears to be primarily yellow-orange, indicative of an older stellar population with a reduced rate of ongoing star formation. There is a very slight flattening or elongation present, hinting at a possible disk component, though the roundness dominates. No significant disturbances or signs of recent or ongoing mergers are apparent in the image. The galaxy appears to be relatively isolated and unperturbed.
