The galaxy presents as a centrally concentrated, luminous object. Its morphology is predominantly smooth, with no discernible spiral arms or bar structure visible at this resolution. The color profile appears to exhibit a radial gradient, transitioning from a yellowish-white core to a redder halo. The overall shape is nearly round, suggesting a possible elliptical or S0 classification. There is a subtle indication of minor disturbances in the outer regions, possibly hinting at past interactions or mergers, but these are not pronounced. The galaxy exhibits a measurable redshift, indicating it resides at a significant cosmological distance. Star formation activity appears to be present, albeit at a relatively low level, consistent with the smooth morphology.
