The galaxy presents a generally smooth and rounded morphology. Its light profile appears relatively concentrated, with a bright, yellowish core that diminishes gradually towards the outer regions. There is little evidence of distinct spiral arms or a prominent disk structure. The color suggests a stellar population with a mix of ages, with a higher concentration of older stars in the central region. No significant tidal disturbances or merging features are discernible in the immediate vicinity of the galaxy. The object appears to be a relatively quiescent system with low ongoing star formation activity.
