The galaxy presents as a single, largely homogenous body of light. Its overall form is elliptical, exhibiting a high degree of central concentration. The light distribution appears smooth, with no obvious spiral arm structures or distinct clumps of star formation visible. Color gradients across the galaxy are subtle, with a general trend toward redder hues. Based on its features, the galaxy appears to be a relatively old system, possibly a spheroid galaxy. There is no apparent dust absorption or ongoing star formation, suggesting a quiescent state. Overall, this galaxy is consistent with a well-evolved system dominated by older stellar populations.
