The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a spheroidal morphology with a notable lack of distinct spiral arms or a prominent disk structure. The color profile is dominated by yellowish hues, suggesting a population of older stars and/or a significant dust component absorbing bluer wavelengths of light. The overall shape is generally round, with a slight hint of elongation, although it is difficult to ascertain the exact ellipticity. There is no clear evidence of any major merging activity or significant tidal disturbances in the immediate vicinity. The galaxy's central region is noticeably brighter, indicating a concentration of stellar mass toward the core. The outer regions fade gradually into the background, with no sharp cutoff observed.
