The galaxy presents as a moderately luminous, ellipsoidal structure. The central region exhibits a concentrated, bright, yellowish-orange hue, indicative of an older stellar population. Fainter, bluish-green diffuse light is observed surrounding the central region, potentially indicating ongoing, albeit subdued, star formation. The galaxy appears relatively smooth, with a slight elongation suggestive of an elliptical morphology rather than a spiral. There is no clear evidence of a prominent disk structure or significant spiral arm features. A hint of minor tidal disturbance cannot be ruled out, but the overall impression is of a relaxed system. The light distribution falls off gradually from the core, indicating a fairly large effective radius, potentially around 7.8 kiloparsecs. Given its color profile and smooth appearance, this galaxy is probably an elliptical at a redshift of approximately 0.2.
