The galaxy appears as a single, concentrated body of light. Its morphology is predominantly smooth, with a generally elliptical shape that tends towards round, though not perfectly so. There is no clear evidence of spiral arms or a distinct disk-like structure. The color profile suggests a slightly redder hue, indicative of a population of older stars and a low rate of on-going star formation. There is no apparent sign of major mergers or significant tidal disturbances that would disrupt its overall symmetry. Small-scale features are not visible, suggesting that the galaxy is relatively quiescent in terms of recent interaction history. Overall, the galaxy presents as a moderately massive and evolved system, potentially an elliptical galaxy with a somewhat regular form.
